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High-Dimensional Probability and Statistics

Vershynin's High-Dimensional Probability and Wainwright's High-Dimensional Statistics: concentration, random matrices, and sparse recovery.

12 open missions

Missions

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Machine LearningProbabilityRandom Matrix Theory+1·Captain: mikedeng1

High-Dimensional Probability IV: Norms of Random Matrices with Sub-gaussian EntriesTextbook

Motivation

Random matrices with independent entries appear whenever a system is measured through many noisy, roughly independent channels: shot noise in a sensor array, edges in an Erdős–Rényi-type random graph, or the design matrix of a linear model with independent covariates. A basic question about any such matrix AAA is how far it can stretch a vector — its operator norm ∥A∥\|A\|∥A∥ — since this single number controls the stability of every linear statistic computed from AAA: least-squares estimates, spectral clustering, covariance estimation, and random projections all reduce, at some point, to bounding ∥A∥\|A\|∥A∥.

The theory traces to Marchenko and Pastur's 1967 asymptotic law for the spectrum of large random matrices, and to Bai and Yin's 1988 almost-sure limit ∥A∥/n→2\|A\|/\sqrt n \to 2∥A∥/n​→2 for n×nn \times nn×n matrices with i.i.d. mean-zero, unit-variance entries. Those results are asymptotic: they say what happens as the dimension n→∞n \to \inftyn→∞, for a fixed matrix shape. The result formalized here, Theorem 4.4.5 of Vershynin's High-Dimensional Probability (2018) (DOI 10.1017/9781108231596), belongs to the more recent non-asymptotic strand of the theory: it gives an explicit, dimension-free bound that holds at every fixed m,nm, nm,n, with an explicit failure probability — the form of statement needed for finite-sample guarantees in statistics and data science, rather than limiting behavior.

Setting

Let AAA be an m×nm \times nm×n real matrix. Equip Rn\mathbb R^nRn and Rm\mathbb R^mRm with the Euclidean norm ∥⋅∥2\|\cdot\|_2∥⋅∥2​; AAA acts as a linear map ℓ2n→ℓ2m\ell_2^n \to \ell_2^mℓ2n​→ℓ2m​. Its operator norm (§4.1.2) is

∥A∥  :=  max⁡x∈Sn−1∥Ax∥2,\|A\| \;:=\; \max_{x \in S^{n-1}} \|Ax\|_2 ,∥A∥:=x∈Sn−1max​∥Ax∥2​,

the largest factor by which AAA can stretch a unit vector; equivalently, the largest singular value of AAA.

A real random variable XXX is sub-gaussian with the mission's own convention (matching the Orlicz ψ2\psi_2ψ2​ norm this series already carries as a published definition, HighDimProb.Concentration.subgaussianNorm) if

∥X∥ψ2  :=  inf⁡{t>0:Eexp⁡(X2/t2)≤2}  <  ∞.\|X\|_{\psi_2} \;:=\; \inf\{t > 0 : \mathbb E \exp(X^2/t^2) \le 2\} \;<\; \infty .∥X∥ψ2​​:=inf{t>0:Eexp(X2/t2)≤2}<∞.

Bounded random variables and Gaussians are sub-gaussian; a Bernoulli(ppp) variable and a ±1\pm 1±1-valued coin flip both qualify, which is why the theorem below directly covers random matrices with i.i.d. Rademacher or Gaussian entries as special cases.

The mission's proof technique is the ε-net argument, developed in §4.2 and used nowhere before this chapter of the book: a metric space (T,d)(T,d)(T,d), a subset K⊆TK \subseteq TK⊆T, and ε>0\varepsilon > 0ε>0 give rise to an ε-net N⊆KN \subseteq KN⊆K — a finite set such that every point of KKK is within ε\varepsilonε of some point of NNN — and a covering number N(K,d,ε)N(K, d, \varepsilon)N(K,d,ε), the smallest cardinality of such a net. The technique reduces a statement that must hold uniformly over an infinite (compact) set to a statement about finitely many points, paid for by a union bound whose cost is controlled by the covering number.

Formalization targets

Goal (Theorem 4.4.5)

∃ C>0  such that  ∀ t>0,Prob{ ∥A∥≤CK(m+n+t) }  ≥  1−2exp⁡(−t2),\exists\, C > 0 \;\text{such that}\; \forall\, t > 0,\quad \mathrm{Prob}\bigl\{\, \|A\| \le CK(\sqrt m + \sqrt n + t) \,\bigr\} \;\ge\; 1 - 2\exp(-t^2),∃C>0such that∀t>0,Prob{∥A∥≤CK(m​+n​+t)}≥1−2exp(−t2),

for any m×nm \times nm×n random matrix AAA with independent, mean-zero, sub-gaussian entries AijA_{ij}Aij​ and K=max⁡i,j∥Aij∥ψ2K = \max_{i,j} \|A_{ij}\|_{\psi_2}K=maxi,j​∥Aij​∥ψ2​​. This is the weakest stable form of the bound — it fixes no numerical value for CCC, only its existence and absoluteness (independence from mmm, nnn, AAA, ttt), so later refinements of the constant do not invalidate it.

Significance

The result itself. The bound ∥A∥≲m+n\|A\| \lesssim \sqrt m + \sqrt n∥A∥≲m​+n​ is sharp up to the constant: for entries of unit variance, E∥A∥≥14(m+n)\mathbb E\|A\| \ge \tfrac14(\sqrt m + \sqrt n)E∥A∥≥41​(m​+n​) for large m,nm, nm,n (the book's Exercise 4.4.7), so no non-asymptotic bound of this shape can be improved beyond constants. It is the entry point to the rest of the book's random matrix theory: Corollary 4.4.8 specializes it to symmetric matrices, and it underlies the community-detection (§4.5) and covariance-estimation (§4.7) applications later in the same chapter, neither of which is part of this mission.

Formalizing it. The theorem is a classical, fully proved result; nothing about its truth is open. What this mission contributes is a machine-checked formal statement — together with the two pieces of chapter infrastructure its own textbook proof names by number (Corollary 4.2.13, Exercise 4.4.3(a)) — and a third, self-contained application of the same covering-number machinery (Theorem 4.3.5) that exercises the shared IsEpsNet/coveringNumber definitions on a different metric space (the Hamming cube), independently of the Euclidean case. Mathlib and the Prove2Me platform currently have no ε-net, covering-number, or packing-number infrastructure (checked by q=random matrix, q=operator norm, q=covering number, q=net on the platform, and by filename search in Mathlib): this mission is the first to introduce it, restated inside its own namespace since it is not otherwise available to build on.

Difficulty

The obvious first approach is to bound ∥A∥=max⁡x∈Sn−1∥Ax∥2\|A\| = \max_{x \in S^{n-1}} \|Ax\|_2∥A∥=maxx∈Sn−1​∥Ax∥2​ directly by union-bounding a concentration inequality over the sphere Sn−1S^{n-1}Sn−1. This fails outright: Sn−1S^{n-1}Sn−1 is infinite (indeed uncountable) for n≥2n \ge 2n≥2, so no union bound over its points can converge — the naive approach gives ∞⋅(tail probability)\infty \cdot (\text{tail probability})∞⋅(tail probability). The ε-net argument is the fix, but it is not just "discretize and hope": the reduction from the sphere to a finite net (quadratic_form_on_net, Exercise 4.4.3(a)) loses a multiplicative factor 1/(1−2ε)1/(1-2\varepsilon)1/(1−2ε) that must be tracked, and the net's cardinality (covering_numbers_of_euclidean_ball_and_sphere, Corollary 4.2.13) is exponential in the dimension (9n9^n9n at ε=1/4\varepsilon = 1/4ε=1/4) — so the per-point tail probability from Hoeffding-type concentration must itself decay fast enough (quadratically in the exponent) to survive multiplying by 9m+n9^{m+n}9m+n many points. Getting the union bound to close requires choosing the threshold uuu in the tail bound proportionally to m+n+t\sqrt m + \sqrt n + tm​+n​+t, not to ttt alone — the m+n\sqrt m + \sqrt nm​+n​ term is exactly what pays for the net's exponential size.

Formalization scope

AAA is represented as Ω → Matrix (Fin m) (Fin n) ℝ; its entries A ω i j are the individual real random variables. Independence of the mnmnmn entries is iIndepFun over the index type Fin m × Fin n; mean-zero is the vanishing of each entry's Bochner integral. The operator norm is the norm of the associated continuous linear map between EuclideanSpace ℝ (Fin n) and EuclideanSpace ℝ (Fin m) (matrixOpNorm, every linear map between finite-dimensional normed spaces being automatically continuous), matching the book's maxₓ∈Sⁿ⁻¹ ‖Ax‖₂ exactly. The sub-gaussian norm KKK reuses this series' own published definition, HighDimProb.Concentration.subgaussianNorm, rather than a re-derivation. Covering numbers (coveringNumber) are restricted to finite (Finset) ε-nets, the only kind this chapter uses; this is a deliberate restriction, not a general-purpose covering-number formalization, and is disclosed as such. A hard-coded numeral for CCC, or an unquantified "with high probability" in place of the explicit failure probability 2exp⁡(−t2)2\exp(-t^2)2exp(−t2), would each trivialize the statement and is ruled out: CCC is existentially bound ahead of every other quantifier, and t>0t > 0t>0 is a free parameter with its own explicit bound, exactly as the book states it.

Definitions reusable beyond this mission: IsEpsNet and coveringNumber are stated for a general PseudoMetricSpace and apply unchanged to any later chapter's covering-number needs (e.g. Chapter 8's VC-dimension covering numbers), though per this series' rule that drafts cannot import drafts, a later chunk would restate rather than import them until this mission is published. matrixOpNorm is likewise chapter-agnostic. Contributions completing the sorry proofs of any of the four theorem items are welcome and independent of one another; the covering number and net-reduction items (covering_numbers_of_euclidean_ball_and_sphere, quadratic_form_on_net) are the standard prerequisites for the goal's own volumetric/ε-net proof.

Selected references

  • Vershynin, R. High-Dimensional Probability: An Introduction with Applications in Data Science. Cambridge University Press, 2018. DOI 10.1017/9781108231596
  • Bai, Z. D., Yin, Y. Q. "Necessary and sufficient conditions for almost sure convergence of the largest eigenvalue of a Wigner matrix." Annals of Probability 16 (1988), 1729–1741.
  • Marchenko, V. A., Pastur, L. A. "Distribution of eigenvalues for some sets of random matrices." Mathematics of the USSR-Sbornik 1 (1967), 457–483.
12 thms4 active users
Machine LearningProbabilityStatistics·Captain: mikedeng1

High-Dimensional Statistics III: A Uniform Law via Rademacher ComplexityTextbook

Motivation

Many statistical estimators are defined by minimizing an empirical average over a class of candidate models — empirical risk minimization, maximum likelihood, and binary classification all fit this template. Analyzing such an estimator's excess risk reduces, in each case, to controlling how far the empirical average of a whole class of functions can deviate from its population expectation, not just a single fixed function — a much stronger requirement than the ordinary law of large numbers, which only controls one function at a time. This mission formalizes the central non-asymptotic tool for this problem, the Rademacher complexity-based uniform law, following Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint (Cambridge University Press, 2019), Chapter 4.

Setting

Let FFF be a class of real-valued functions with a common domain, indexed as F={fj,j∈ι}F=\{f_j, j\in\iota\}F={fj​,j∈ι}, and let X1,…,XnX_1,\dots,X_nX1​,…,Xn​ be i.i.d. samples from a distribution PPP. The empirical process deviation (Eq. (4.7)) is

∥Pn−P∥F  :=  sup⁡f∈F∣1n∑i=1nf(Xi)−E[f(X)]∣.\|\mathbb P_n-P\|_F \;:=\; \sup_{f\in F}\Big|\frac1n\sum_{i=1}^n f(X_i) - \mathbb E[f(X)]\Big|.∥Pn​−P∥F​:=f∈Fsup​​n1​i=1∑n​f(Xi​)−E[f(X)]​.

Given an independent Rademacher sequence ε1,…,εn\varepsilon_1,\dots,\varepsilon_nε1​,…,εn​ (each εi=±1\varepsilon_i=\pm1εi​=±1 equiprobably), the symmetrized process (Eq. (4.19)) and the Rademacher complexity (Eq. (4.13)) of FFF are

∥Sn∥F:=sup⁡f∈F∣1n∑i=1nεif(Xi)∣,Rn(F):=EX,ε[∥Sn∥F].\|S_n\|_F := \sup_{f\in F}\Big|\frac1n\sum_{i=1}^n\varepsilon_if(X_i)\Big|, \qquad R_n(F) := \mathbb E_{X,\varepsilon}[\|S_n\|_F].∥Sn​∥F​:=f∈Fsup​​n1​i=1∑n​εi​f(Xi​)​,Rn​(F):=EX,ε​[∥Sn​∥F​].

A class FFF is bbb-uniformly bounded if ∥f∥∞≤b\|f\|_\infty\le b∥f∥∞​≤b for every f∈Ff\in Ff∈F.

Formalization targets

Goal — Theorem 4.10 (a uniform law via Rademacher complexity)

For any bbb-uniformly bounded class FFF, any n≥1n\ge1n≥1, and any δ≥0\delta\ge0δ≥0,

∥Pn−P∥F  ≤  2Rn(F)+δ\|\mathbb P_n-P\|_F \;\le\; 2R_n(F)+\delta∥Pn​−P∥F​≤2Rn​(F)+δ

with PPP-probability at least 1−exp⁡(−nδ2/2b2)1-\exp(-n\delta^2/2b^2)1−exp(−nδ2/2b2).

Milestone — Proposition 4.11 (symmetrization sandwich)

For any convex non-decreasing Φ\PhiΦ, E[Φ(12∥Sn∥Fˉ)]≤E[Φ(∥Pn−P∥F)]≤E[Φ(2∥Sn∥F)]\mathbb E[\Phi(\tfrac12\|S_n\|_{\bar F})] \le \mathbb E[\Phi(\|\mathbb P_n-P\|_F)] \le \mathbb E[\Phi(2\|S_n\|_F)]E[Φ(21​∥Sn​∥Fˉ​)]≤E[Φ(∥Pn​−P∥F​)]≤E[Φ(2∥Sn​∥F​)], where Fˉ\bar FFˉ is the recentered class. This generalizes the specific symmetrization step used in Theorem 4.10's own proof (the case Φ(t)=t\Phi(t)=tΦ(t)=t) to an entire family of moment comparisons.

Milestone — Eq. (4.16) (concentration around the mean)

For a bbb-uniformly bounded, i.i.d.-sampled class FFF, ∥Pn−P∥F−E[∥Pn−P∥F]≤t\|\mathbb P_n-P\|_F - \mathbb E[\|\mathbb P_n-P\|_F] \le t∥Pn​−P∥F​−E[∥Pn​−P∥F​]≤t with PPP-probability at least 1−e−nt2/2b21-e^{-nt^2/2b^2}1−e−nt2/2b2, obtained via the bounded-differences method. Combined with Proposition 4.11's bound on E[∥Pn−P∥F]\mathbb E[\|\mathbb P_n-P\|_F]E[∥Pn​−P∥F​] by 2Rn(F)2R_n(F)2Rn​(F), this is exactly Theorem 4.10's proof.

Significance

Theorem 4.10 is the general-purpose engine behind the classical Glivenko–Cantelli theorem (recovered by taking FFF to be the class of half-line indicator functions, Example 4.6) and behind uniform convergence guarantees for empirical risk minimization more broadly (Section 4.1.2): whenever a task can be reduced to bounding the Rademacher complexity of a specific function class — a purely combinatorial/geometric quantity independent of any particular statistical model — Theorem 4.10 converts that bound directly into a high-probability uniform convergence guarantee. Proposition 4.11 is separately significant as the general symmetrization principle from which Theorem 4.10's specific bound, and many similar bounds throughout empirical process theory, are instances.

Formalizing it. No faithful prior art exists on the platform: a fresh search for "uniform law," "symmetrization," "Rademacher complexity," "Glivenko-Cantelli," and "empirical process" found only unrelated hits and the existing RademacherSymmetrization.*/RademacherMassart.* items, which are specific to finite function classes (Finset (X → ℝ)) — a strictly narrower setting than Theorem 4.10's fully general (possibly infinite) function classes, and not reused here. All three theorems are drafted as open goals (:= by sorry).

Difficulty

The naive approach to bounding ∥Pn−P∥F\|\mathbb P_n-P\|_F∥Pn​−P∥F​ — apply a scalar concentration bound to each f∈Ff\in Ff∈F individually and union-bound over FFF — fails outright when FFF is infinite (there is no union bound to take). The two-step resolution captured by this mission's milestones avoids this entirely: first, ∥Pn−P∥F\|\mathbb P_n-P\|_F∥Pn​−P∥F​ itself, viewed as a single function of the nnn samples, is shown to concentrate sharply around its own mean via the bounded-differences method (no union bound over FFF needed — the argument treats sup⁡f∈F(⋯ )\sup_{f\in F}(\cdots)supf∈F​(⋯) as one Lipschitz function of the samples). Second, the mean E[∥Pn−P∥F]\mathbb E[\|\mathbb P_n-P\|_F]E[∥Pn​−P∥F​] itself, a single deterministic number, is bounded via symmetrization: introducing an independent "ghost sample" YiY_iYi​ with the same law as XiX_iXi​ converts the un-symmetric quantity E[sup⁡f∣(1/n)∑f(Xi)−Ef∣]\mathbb E[\sup_f|(1/n)\sum f(X_i)-\mathbb E f|]E[supf​∣(1/n)∑f(Xi​)−Ef∣] into the manifestly symmetric E[sup⁡f∣(1/n)∑εi(f(Xi)−f(Yi))∣]\mathbb E[\sup_f|(1/n)\sum\varepsilon_i (f(X_i)-f(Y_i))|]E[supf​∣(1/n)∑εi​(f(Xi​)−f(Yi​))∣], and it is only after this symmetrization that the supremum over FFF becomes tractable via the geometry of FFF (its Rademacher complexity) rather than requiring FFF finite.

Formalization scope

The function class FFF is realized as the range of an index family f:ι→D→Rf:\iota\to D\to\mathbb Rf:ι→D→R rather than a Set (D → ℝ), matching the standard representation of a (possibly infinite) function class by an index type; ι carries no finiteness assumption, matching the book's own full generality (in contrast to the platform's existing RademacherSymmetrization/ RademacherMassart items, which are finite-class-specific). The population expectation E[f(X)]\mathbb E[f(X)]E[f(X)] is realized via an explicit population variable X0X_0X0​ sharing the samples' common law, rather than a separately axiomatized abstract distribution object. The Rademacher sequence and the samples are packaged into one jointly independent family Z : ℕ → Ω → D × ℝ with an explicit hypothesis that the two coordinates are themselves independent at each index — capturing "ε\varepsilonε independent of XXX, both i.i.d." exactly, without a bespoke joint-independence predicate.

Theorem 4.10's own qualitative corollary ("consequently, ∥Pn−P∥F→a.s.0\|\mathbb P_n-P\|_F\xrightarrow{a.s.}0∥Pn​−P∥F​a.s.​0 whenever Rn(F)=o(1)R_n(F)=o(1)Rn​(F)=o(1)") is not included in the goal's conclusion: it concerns an infinite sequence of samples and asymptotic convergence via the Borel–Cantelli lemma, a substantially different formal object (requiring Filter.Tendsto over ℕ→∞ and ∀ᵐ almost-sure convergence) from the single-nnn non-asymptotic tail bound (4.14) this mission's goal states, and is left as natural follow-on work, alongside a direct formalization of the classical Glivenko–Cantelli theorem (Theorem 4.4) as a corollary.

Lemma 4.14 (the polynomial-discrimination route to bounding Rademacher complexity for VC-type classes) is out of scope for this mission: its displayed inequality is extracted with heavily garbled math layout from the source PDF (a known, disclosed limitation of this book's text extraction at that specific page), and confirming it character-for-character against the rendered page image was judged out of budget for this chunk relative to Proposition 4.11 and Eq. (4.16), both of which are directly load-bearing in Theorem 4.10's own proof and extracted cleanly.

Selected references

  • M. J. Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint, Cambridge University Press, 2019. DOI: 10.1017/9781108627771. Chapter 4.
  • M. Ledoux and M. Talagrand, Probability in Banach Spaces: Isoperimetry and Processes, Springer, 1991 (the symmetrization technique).
  • V. N. Vapnik and A. Y. Chervonenkis, "On the uniform convergence of relative frequencies of events to their probabilities," Theory of Probability and Its Applications, 16(2):264–280, 1971.
9 thms3 active usersReviewed
Machine LearningProbabilityRandom Matrix Theory+2·Captain: mikedeng1

High-Dimensional Probability VIII: Dudley's Integral InequalityTextbook

Motivation

Many questions in high-dimensional probability reduce to bounding the expected supremum of a random process (Xt)t∈T(X_t)_{t\in T}(Xt​)t∈T​ — the maximum, over an entire indexed family of random variables, of how large any one of them can get. When TTT is finite this is routine (a union bound over ∣T∣|T|∣T∣ terms suffices), but the interesting cases have TTT infinite, even uncountable: a supremum over a continuum of test functions, a norm expressed as a supremum over a sphere, or an empirical process indexed by a whole class of functions. A naive union bound is unusable here, since ∣T∣|T|∣T∣ is infinite.

R. M. Dudley's 1967 entropy bound (R. M. Dudley, The sizes of compact subsets of Hilbert space and continuity of Gaussian processes, Journal of Functional Analysis 1 (1967), 290–330) resolved this for Gaussian processes, controlling the expected supremum purely in terms of the metric entropy of TTT — how many balls of radius ε\varepsilonε are needed to cover TTT, at every scale ε\varepsilonε. The technique behind the proof, chaining, builds a sequence of increasingly fine finite approximations to TTT and telescopes the resulting bounds; it is one of the central tools of the field, reused throughout empirical process theory, statistical learning theory (via Vapnik-Chervonenkis theory), and non-asymptotic random matrix theory. This mission formalizes the chapter's generalization of Dudley's bound beyond Gaussian processes, to any process with sub-gaussian increments, together with the purely combinatorial Sauer-Shelah lemma that the chapter's applications to statistical learning theory build on.

Setting

Fix a probability space (Ω,F,P)(\Omega,\mathcal F,P)(Ω,F,P). A random process is a family (Xt)t∈T(X_t)_{t\in T}(Xt​)t∈T​ of real random variables on (Ω,F,P)(\Omega,\mathcal F,P)(Ω,F,P) indexed by an arbitrary set TTT, with no independence or measurability-of-the-supremum assumed between different ttt's. Since sup⁡t∈TXt(ω)\sup_{t\in T}X_t(\omega)supt∈T​Xt​(ω) need not be measurable in ω\omegaω for a general index set TTT, its expectation is understood — following the book's own convention, set once in Chapter 7 and reused throughout — through the process's finite-dimensional marginals:

Esup⁡t∈TXt  :=  sup⁡T0⊆T finite, nonempty Emax⁡t∈T0Xt.\mathbb E\sup_{t\in T}X_t \;:=\; \sup_{T_0\subseteq T\text{ finite, nonempty}}\ \mathbb E\max_{t\in T_0}X_t.Et∈Tsup​Xt​:=T0​⊆T finite, nonemptysup​ Et∈T0​max​Xt​.

Now fix a metric ddd on TTT, making (T,d)(T,d)(T,d) a metric space. The covering number N(T,d,ε)N(T,d,\varepsilon)N(T,d,ε), for ε>0\varepsilon>0ε>0, is the smallest cardinality of a finite ε\varepsilonε-net of TTT: a finite set N⊆TN\subseteq TN⊆T such that every point of TTT lies within distance ε\varepsilonε of some point of NNN (or N(T,d,ε):=∞N(T,d,\varepsilon):=\inftyN(T,d,ε):=∞ if no finite ε\varepsilonε-net exists). The quantity log⁡N(T,d,ε)\log N(T,d,\varepsilon)logN(T,d,ε) is the metric entropy of TTT at scale ε\varepsilonε: it measures how large TTT looks when resolved only down to scale ε\varepsilonε.

A process (Xt)t∈T(X_t)_{t\in T}(Xt​)t∈T​ has sub-gaussian increments with parameter K≥0K\ge0K≥0 if

∥Xt−Xs∥ψ2  ≤  K d(t,s)for all t,s∈T,\|X_t-X_s\|_{\psi_2}\;\le\;K\,d(t,s)\qquad\text{for all }t,s\in T,∥Xt​−Xs​∥ψ2​​≤Kd(t,s)for all t,s∈T,

where ∥⋅∥ψ2\|\cdot\|_{\psi_2}∥⋅∥ψ2​​ is the sub-gaussian (Orlicz) norm of Chapter 2: the smallest u>0u>0u>0 with Eexp⁡((Xt−Xs)2/u2)≤2\mathbb E\exp((X_t-X_s)^2/u^2)\le2Eexp((Xt​−Xs​)2/u2)≤2. This says the increments of the process are controlled by the metric ddd the way a Gaussian process's increments are controlled by its own canonical metric d(t,s):=∥Xt−Xs∥L2d(t,s):=\|X_t-X_s\|_{L^2}d(t,s):=∥Xt​−Xs​∥L2​ — but without assuming (Xt)t∈T(X_t)_{t\in T}(Xt​)t∈T​ is Gaussian.

A class of Boolean functions FFF on a set Ω\OmegaΩ shatters a subset Λ⊆Ω\Lambda\subseteq\OmegaΛ⊆Ω if every function g:Λ→{0,1}g:\Lambda\to\{0,1\}g:Λ→{0,1} arises as the restriction to Λ\LambdaΛ of some f∈Ff\in Ff∈F. The VC (Vapnik-Chervonenkis) dimension vc(F)\mathrm{vc}(F)vc(F) is the largest cardinality of a subset of Ω\OmegaΩ shattered by FFF (or ∞\infty∞ if arbitrarily large finite subsets, or an infinite one, are shattered) — a purely combinatorial measure of how rich the class FFF is.

Formalization targets

Goal (Theorem 8.1.3, Dudley's integral inequality)

∃ C>0:Esup⁡t∈TXt  ≤  CK∫0∞log⁡N(T,d,ε)  dε\exists\,C>0:\quad\mathbb E\sup_{t\in T}X_t\;\le\;CK\int_0^\infty\sqrt{\log N(T,d,\varepsilon)}\;d\varepsilon∃C>0:Et∈Tsup​Xt​≤CK∫0∞​logN(T,d,ε)​dε

for every mean-zero random process (Xt)t∈T(X_t)_{t\in T}(Xt​)t∈T​ on a metric space (T,d)(T,d)(T,d) with sub-gaussian increments parameter K≥0K\ge0K≥0, whenever the integral is finite. CCC is the book's own unnamed absolute constant, never depending on TTT, KKK, or the process. This is the weakest stable form of the claim: no numeral is hard-coded for CCC, and the statement asks only for the shape of the bound, matching what the book actually proves.

Milestone (Theorem 8.3.16, Sauer-Shelah lemma)

∣F∣  ≤  ∑k=0d(nk)  ≤  (end)d,d:=vc(F),|F|\;\le\;\sum_{k=0}^{d}\binom nk\;\le\;\left(\frac{en}{d}\right)^{d},\qquad d:=\mathrm{vc}(F),∣F∣≤k=0∑d​(kn​)≤(den​)d,d:=vc(F),

for every class FFF of Boolean functions on a finite nnn-point set Ω\OmegaΩ. This is a purely combinatorial fact, with no probability involved, but it is the bridge (via the covering-number bound Theorem 8.3.18, outside this mission's scope) between the chapter's Dudley-inequality engine and its statistical-learning applications — a bound on how large a finite class of Boolean functions can be, in terms of a single combinatorial complexity parameter.

Significance

Dudley's inequality is, in the book's own words, "the main result" of the chaining chapter: it converts a purely geometric quantity — the metric entropy of an index set, computable in many cases from covering-number estimates already available for balls, ellipsoids, and other convex bodies — into a probabilistic control on the size of a random process indexed by that set. This is what lets later chapters (uniform laws of large numbers over function classes, the matrix deviation inequality, the Dvoretzky-Milman theorem on almost-spherical sections of convex bodies) bound suprema over infinite, even uncountable, index sets without ever performing a union bound. The bound is also known to be tight only up to a logarithmic factor in general — Sudakov's minoration inequality (Chapter 7) gives a matching lower bound for Gaussian processes, and the book's own Exercise 8.1.12 exhibits a set where the two bounds genuinely diverge — so the constant CCC here cannot in general be sharpened away.

The Sauer-Shelah lemma is one of the two founding results of VC theory (together with the Glivenko-Cantelli-type uniform convergence it feeds into), independently discovered by Vapnik and Chervonenkis, Sauer, and Shelah in the early 1970s; it underlies the sample-complexity bounds of statistical learning theory (a hypothesis class with finite VC dimension is PAC-learnable) and, through Theorem 8.3.18, gives one of the two standard routes (the other being direct combinatorial counting) to bounding covering numbers of infinite function classes.

Both results are decades old and have long-established, standard proofs; no open mathematical question is being formalized. What this mission contributes is the machine-checked statement infrastructure — the goal and the Sauer-Shelah milestone, together with the definitions (CoveringNumber, ProcessESup, Shatters, VcDim) a faithful Lean rendering of either result needs — for a solver to close with a proof. No formalization of Dudley's inequality or the Sauer-Shelah lemma is known to exist on the platform prior to this mission.

Difficulty

The natural first idea for bounding Esup⁡t∈TXt\mathbb E\sup_{t\in T}X_tEsupt∈T​Xt​ is a single-scale ε\varepsilonε-net argument: replace TTT by a finite ε\varepsilonε-net, bound the maximum over the (finite) net by a union bound using the sub-gaussian tail, and separately bound the error of replacing TTT by the net using the Lipschitz-in-probability control the sub-gaussian-increments hypothesis gives. This works, but it only ever sees TTT at one fixed resolution ε\varepsilonε, and optimizing over ε\varepsilonε afterward gives a bound with an extra log⁡(1/ε)\sqrt{\log(1/\varepsilon)}log(1/ε)​-type loss that does not match Dudley's inequality. The actual difficulty is genuinely multi-scale: chaining builds a whole sequence of nets at dyadic scales ε=2−k\varepsilon=2^{-k}ε=2−k simultaneously, connects each point of TTT to its nearest net point at every scale to form a "chain" of successive approximations back to a single fixed basepoint, and telescopes the resulting sum of increments — turning XtX_tXt​ itself into a sum of differences between successive links of the chain, each individually well controlled by the sub-gaussian hypothesis at its own scale. Passing from the resulting discrete sum over dyadic scales (Theorem 8.1.4) to the continuous integral of the goal is a further, separate technical step.

For the Sauer-Shelah lemma, the natural first idea — bound ∣F∣|F|∣F∣ directly by counting — has no obvious purchase on an arbitrary class of Boolean functions. The actual argument goes through Pajor's lemma, which reduces bounding ∣F∣|F|∣F∣ to counting the shattered subsets of Ω\OmegaΩ instead of the functions in FFF themselves; only then does the cardinality bound d=vc(F)d=\mathrm{vc}(F)d=vc(F) on shattered sets become directly usable, via a binomial-sum estimate.

Formalization scope

CoveringNumber T ε is ℕ∞-valued (ℕ∞ = WithTop ℕ), defined as the infimum, over the subtype of finite ε\varepsilonε-nets of the whole type T (an instance of MetricSpace T), of their cardinality; the infimum of the empty family in this complete lattice is ⊤, reproducing "N:=∞N:= \inftyN:=∞ if no finite net exists" with no case split. ProcessESup is EReal-valued, defined as the supremum over finite nonempty T0⊆TT_0\subseteq TT0​⊆T of the Bochner integral of the finite max — EReal, not ℝ, because a real-valued supremum would silently return the junk value 000 if the family of marginal expectations were unbounded above. Shatters and VcDim are direct transcriptions of Definition 8.3.1, with VcDim valued in ℕ∞ via a supremum of Set.encard over the (always-nonempty, since ∅\varnothing∅ is trivially shattered) subtype of shattered subsets. The goal's mean-zero hypothesis is stated as Integrable (X t) P ∧ ∫ X t = 0 rather than the bare equation, since a non-integrable variable's Bochner integral is 0 in Mathlib by convention regardless of its true mean — a bare-equation hypothesis would let a non-mean-zero, non-integrable process satisfy the theorem vacuously. Two further hypotheses make explicit what the book's own displayed statement treats as understood without spelling out: that N(T,d,ε)N(T,d,\varepsilon)N(T,d,ε) is finite for every ε>0\varepsilon>0ε>0 (total boundedness of TTT), and that the resulting integrand is integrable on (0,∞)(0,\infty)(0,∞) — both hold whenever TTT is totally bounded, since the integrand vanishes once ε≥diam(T)\varepsilon\ge\mathrm{diam}(T)ε≥diam(T), so neither hypothesis excludes any case the book's own proof does not also need. [Nonempty T] excludes the degenerate empty index set. The absolute constant CCC is existentially quantified ahead of every type, instance, and hypothesis it is uniform over, and pinned to no numeral, matching "CCC is an absolute constant" — a formalization hard-coding a specific numeral for CCC would be invalidated by the next sharper constant in the literature and would not match what the book proves.

A trivializing formalization of the Sauer-Shelah lemma would fix vc(F)\mathrm{vc}(F)vc(F) at a hard-coded small value, or drop the second (exponential) inequality in favor of the weaker first one; this mission's statement keeps both inequalities, with ddd genuinely computed from VcDim, and handles the d=0d=0d=0 boundary (where the exponential bound's base involves a division by zero under Lean's x/0=0 convention) explicitly rather than excluding it, since x^0=1 still recovers the book's correct bound ∣F∣≤1|F|\le1∣F∣≤1 there.

This mission covers Theorem 8.1.3 and Theorem 8.3.16 only; Theorem 8.3.18 (covering numbers via VC dimension) and Theorem 8.2.3 (the uniform law of large numbers, the chapter's direct application of Dudley's inequality) are left out, not approximated, for lack of the additional empirical- process measurability machinery — the class of Lipschitz functions of Eq. (8.22), measurability of the resulting empirical process — that a faithful statement of either would need beyond what this mission's items already provide. CoveringNumber and ProcessESup are reusable by any later chapter needing a metric space's covering numbers or a general random process's expected supremum (this book's own Chapters 7, 9, and 11 all use one or both); Shatters and VcDim are reusable by any later development of VC theory or statistical learning theory. Solvers' contributions are welcome on: the chaining argument itself (the mission's hardest open leaf, via the discrete dyadic form of Theorem 8.1.4), Pajor's lemma underlying Sauer-Shelah, and the binomial-sum estimate closing its second inequality.

Selected references

  • R. M. Dudley, The sizes of compact subsets of Hilbert space and continuity of Gaussian processes, Journal of Functional Analysis 1 (1967), 290–330. https://doi.org/10.1016/0022-1236(67)90017-1
  • N. Sauer, On the density of families of sets, Journal of Combinatorial Theory, Series A 13 (1972), 145–147. https://doi.org/10.1016/0097-3165(72)90019-2
  • V. N. Vapnik, A. Ya. Chervonenkis, On the uniform convergence of relative frequencies of events to their probabilities, Theory of Probability & Its Applications 16 (1971), 264–280. https://doi.org/10.1137/1116025
  • R. Vershynin, High-Dimensional Probability: An Introduction with Applications in Data Science, Cambridge University Press, 2018, Chapter 8. https://doi.org/10.1017/9781108231596
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Machine LearningProbabilityRandom Matrix Theory+1·Captain: mikedeng1

High-Dimensional Probability IX: The Matrix Deviation InequalityTextbook

Motivation

Random matrices with independent rows are the workhorse of high-dimensional statistics and compressed sensing: sample covariance matrices, sub-sampled measurement operators, and randomized sketches are all of this form. A basic question about such a matrix AAA is how close ∥Ax∥2\|Ax\|_2∥Ax∥2​ stays to its typical size E∥Ax∥2≈m∥x∥2\mathbb E\|Ax\|_2\approx\sqrt m\|x\|_2E∥Ax∥2​≈m​∥x∥2​ — not just for one fixed xxx, but simultaneously for every xxx in some set TTT of interest (a sphere, a cone, the difference set of a data cloud). A bound that holds only pointwise in xxx is of limited use, since most applications need to reason about the worst case over an entire geometric set at once.

This chapter proves such a uniform bound — the matrix deviation inequality — for matrices with independent, isotropic, sub-gaussian rows, controlling the deviation by a single geometric parameter of TTT, its Gaussian complexity. The result is a direct descendant of the chaining machinery of Chapter 8 (via Talagrand's comparison inequality, Chapter 8.6) and, in this book's own account, subsumes several results proved earlier by other methods — two-sided bounds on random matrices, the Johnson-Lindenstrauss lemma for infinite sets — while also yielding two new consequences central to high-dimensional convex geometry: the M∗M^*M∗ bound and the Escape theorem, both controlling how a random subspace intersects a fixed geometric set.

Setting

Fix a probability space (Ω,F,P)(\Omega,\mathcal F,P)(Ω,F,P). A random vector XXX in Rn\mathbb R^nRn is isotropic if its covariance matrix is the identity, Σ(X)=E[XX⊤]=In\Sigma(X)=\mathbb E[XX^\top]=I_nΣ(X)=E[XX⊤]=In​ — equivalently (the book's own Lemma 3.2.3), E⟨X,x⟩2=∥x∥22\mathbb E\langle X,x\rangle^2=\|x\|_2^2E⟨X,x⟩2=∥x∥22​ for every x∈Rnx\in\mathbb R^nx∈Rn. The sub-gaussian norm of a random vector XXX is ∥X∥ψ2:=sup⁡x∈Sn−1∥⟨X,x⟩∥ψ2\|X\|_{\psi_2}:=\sup_{x\in S^{n-1}}\|\langle X,x\rangle\|_{\psi_2}∥X∥ψ2​​:=supx∈Sn−1​∥⟨X,x⟩∥ψ2​​, the supremum over the unit sphere of the scalar sub-gaussian (Orlicz ψ2\psi_2ψ2​) norm of its one-dimensional marginals; XXX is sub-gaussian when this is finite.

Fix a standard Gaussian random vector g∼N(0,In)g\sim N(0,I_n)g∼N(0,In​) in Rn\mathbb R^nRn (a vector whose coordinates in any orthonormal basis are independent standard normal). For a subset T⊆RnT\subseteq\mathbb R^nT⊆Rn, the Gaussian width and Gaussian complexity of TTT are

w(T):=Esup⁡x∈T⟨g,x⟩,γ(T):=Esup⁡x∈T∣⟨g,x⟩∣,w(T) := \mathbb E\sup_{x\in T}\langle g,x\rangle, \qquad \gamma(T) := \mathbb E\sup_{x\in T}|\langle g,x\rangle|,w(T):=Ex∈Tsup​⟨g,x⟩,γ(T):=Ex∈Tsup​∣⟨g,x⟩∣,

two closely related measures of the geometric size of TTT — "cousins" that agree up to a factor of 222 whenever TTT contains the origin, and agree exactly when TTT is origin-symmetric.

Formalization targets

Goal (Theorem 9.1.1, Matrix deviation inequality)

∃ C>0:Esup⁡x∈T∣ ∥Ax∥2−m∥x∥2 ∣  ≤  CK2γ(T)\exists\,C>0:\quad \mathbb E\sup_{x\in T}\bigl|\,\|Ax\|_2-\sqrt m\|x\|_2\,\bigr| \;\le\; CK^2\gamma(T)∃C>0:Ex∈Tsup​​∥Ax∥2​−m​∥x∥2​​≤CK2γ(T)

for every m×nm\times nm×n matrix AAA whose rows A1,…,AmA_1,\dots,A_mA1​,…,Am​ are independent, isotropic, sub-gaussian random vectors with K:=max⁡i∥Ai∥ψ2K:=\max_i\|A_i\|_{\psi_2}K:=maxi​∥Ai​∥ψ2​​, and every T⊆RnT\subseteq\mathbb R^nT⊆Rn (whenever γ(T)\gamma(T)γ(T) is finite). CCC is the book's own unnamed absolute constant, hard-coded to no numeral — the weakest stable form of the claim.

Milestone (Theorem 9.4.2, the M∗M^*M∗ bound)

E diam(T∩ker⁡A)  ≤  CK2w(T)m\mathbb E\,\mathrm{diam}(T\cap\ker A) \;\le\; \frac{CK^2w(T)}{\sqrt m}Ediam(T∩kerA)≤m​CK2w(T)​

for the same class of matrices AAA and any bounded T⊆RnT\subseteq\mathbb R^nT⊆Rn, where ker⁡A\ker AkerA is the (random) kernel of AAA, a subspace of codimension at most mmm. A direct one-paragraph consequence of the goal theorem (apply it to T−TT-TT−T, then restrict to ker⁡A\ker AkerA, where ∥Ax−Ay∥2\|Ax-Ay\|_2∥Ax−Ay∥2​ vanishes).

Significance

The matrix deviation inequality converts a purely algebraic quantity — how close ∥Ax∥2\|Ax\|_2∥Ax∥2​ stays to m∥x∥2\sqrt m\|x\|_2m​∥x∥2​ — into a single geometric parameter of the index set TTT, letting it subsume, via specializations of TTT, results that were previously proved by separate ad hoc arguments: two-sided singular value bounds on random matrices (TTT a sphere), Johnson-Lindenstrauss-type embeddings for possibly infinite point sets (TTT a difference set), and covariance estimation. The M∗M^*M∗ bound is one of the two classical consequences the book develops fresh from the inequality (the other, the Escape theorem, is outside this mission's scope): it answers, quantitatively, how large a random affine section of a fixed convex body typically is, a question at the heart of the local theory of Banach spaces and of compressed sensing's recovery guarantees (Chapter 10 builds directly on this chapter's machinery). Both results have long-standing, well-understood classical proofs; this mission formalizes their statements, not open research.

Difficulty

The natural first idea — bound ∥Ax∥2−m∥x∥2\|Ax\|_2-\sqrt m\|x\|_2∥Ax∥2​−m​∥x∥2​ pointwise for a fixed xxx using concentration of the norm of a sub-gaussian random vector, then take a union bound over TTT — only works when TTT is finite, and gives a bound that scales with log⁡∣T∣\log|T|log∣T∣ rather than with the actual geometric size of TTT. The book's actual route treats Xx:=∥Ax∥2−m∥x∥2X_x:=\|Ax\|_2-\sqrt m\|x\|_2Xx​:=∥Ax∥2​−m​∥x∥2​, indexed by x∈Rnx\in\mathbb R^nx∈Rn, as a genuine random process and shows it has sub-gaussian increments (∥Xx−Xy∥ψ2≤CK2∥x−y∥2\|X_x-X_y\|_{\psi_2}\le CK^2\|x-y\|_2∥Xx​−Xy​∥ψ2​​≤CK2∥x−y∥2​) — itself a nontrivial fact proved in stages (first for a single unit vector via concentration of the norm, Theorem 3.1.1; then for a pair of unit vectors via a squared-process argument; only then in full generality) — and then invokes Talagrand's comparison inequality (a consequence of the chaining machinery of Chapter 8) to pass from sub-gaussian increments directly to a bound in terms of Gaussian complexity, without ever performing a union bound over TTT itself.

Formalization scope

A is represented by its rows, A : Fin m → Ω → EuclideanSpace ℝ (Fin n), with ‖Ax‖₂ recovered as Real.sqrt (∑ i, ⟨Aᵢ,x⟩²) rather than constructing A as a Matrix/LinearMap — this matches the book's own row-by-row hypotheses exactly and is what both theorems' own proofs use directly. IsIsotropic is formalized via the book's basis-free Lemma 3.2.3 characterization (E⟨X,x⟩² = ‖x‖² for every x) rather than the matrix equation Σ(X)=Iₙ, avoiding a fixed-basis covariance-matrix construction the rest of this chunk's definitions do not otherwise need. SubgaussianVectorNorm reuses the published scalar subgaussianNorm. GaussianWidth and GaussianComplexity realize the standard Gaussian vector g ∼ N(0,Iₙ) as the identity map on Mathlib's own standard Gaussian measure on a finite-dimensional inner product space (ProbabilityTheory.stdGaussian), and both, together with the goal's own left-hand side, use a locally-defined finite-marginal expected-supremum convention (ExpSup, EReal-valued) matching the book's own footnote-3 convention (Section 7.2), reused throughout the series. Both theorems' right-hand sides presuppose their respective geometric parameter (γ(T)\gamma(T)γ(T) or w(T)w(T)w(T)) is a finite real number; since both are EReal-valued in general, each theorem takes an explicit real witness together with a proof that it equals the true value — the same finiteness-disclosure pattern 07-chaining's Dudley inequality uses for its own right-hand integral, needed here for exactly the same reason (the book's own display does not spell out why the quantity is finite, true whenever TTT is bounded, as in every application). CCC (and, in the milestone, the same CCC again — the two are not asserted equal, matching that the book states them as two separate "absolute constants") is existentially quantified before every type, instance and hypothesis it is uniform over. The M∗M^*M∗ bound milestone (m_star_bound) additionally carries the hypothesis m>0m > 0m>0: its conclusion divides by m\sqrt mm​, and without this hypothesis Lean's real-division convention (x/0=0x/0=0x/0=0) makes the right-hand side 000 at m=0m=0m=0 regardless of C,K,w(T)C, K, w(T)C,K,w(T) — false whenever TTT has positive diameter, not merely a weaker or vacuous claim. The book's own proof ("Dividing by m\sqrt mm​ yields …", p. 241) already implicitly assumes m≥1m \ge 1m≥1, matching every other use of mmm in the chapter as a positive count of measurement rows.

A trivializing formalization would fix TTT to be a finite set, collapsing the goal to the elementary union-bound case the book explicitly contrasts its own more general statement against (Section 9.1's opening paragraph: "we may choose an arbitrary subset T⊆RnT\subseteq\mathbb R^nT⊆Rn"); this mission's goal quantifies over an arbitrary Set (EuclideanSpace ℝ (Fin n)) to rule that out.

This mission covers Theorem 9.1.1 and Theorem 9.4.2 only; Theorem 9.4.7 (the Escape theorem) and Theorem 9.2.4 (covariance estimation for lower-dimensional distributions), both named as candidate milestones, are left out for lack of session time given the substantial shared infrastructure this chapter needed from scratch. ExpSup, IsIsotropic, SubgaussianVectorNorm, GaussianWidth and GaussianComplexity are reusable by any later chapter needing an isotropic or sub-gaussian random vector, or a Gaussian-width-type quantity (Chapters 4, 10, 11 of this same book series all use one or more of these notions). Solvers' contributions are welcome on: Theorem 9.1.3 (the sub-gaussian increments of the deviation process, the technical heart of the goal's proof), Talagrand's comparison inequality itself (outside this mission, in 07-chaining's companion chapter), and the one-paragraph reduction from the goal to the M∗M^*M∗ bound.

Selected references

  • S. Mendelson, A. Pajor, N. Tomczak-Jaegermann, Reconstruction and subgaussian operators in asymptotic geometric analysis, Geometric and Functional Analysis 17 (2007), 1248–1282. https://doi.org/10.1007/s00039-007-0618-7
  • V. D. Milman, A new proof of A. Dvoretzky's theorem on cross-sections of convex bodies, Funkcional. Anal. i Priložen. 5 (1971), 28–37.
  • R. Vershynin, High-Dimensional Probability: An Introduction with Applications in Data Science, Cambridge University Press, 2018, Chapter 9. https://doi.org/10.1017/9781108231596
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Machine LearningProbabilityRandom Matrix Theory+1·Captain: mikedeng1

High-Dimensional Probability XI: Dvoretzky-Milman's TheoremTextbook

Motivation

A striking fact discovered by Dvoretzky in the 1960s (conjectured by Grothendieck, and sharpened into its modern quantitative form by Milman in 1971) is that every high-dimensional convex body, however irregular, contains a round slice: a random low-dimensional section (or projection) of any bounded convex set in Rn\mathbb R^nRn is, with high probability, close to a Euclidean ball — provided the dimension of the slice is small enough relative to a single geometric parameter of the body. This is remarkable because it holds for every bounded set, arbitrarily irregular; no special structure is assumed beyond boundedness. This chapter proves the theorem in its Gaussian form, as a culmination of every geometric and probabilistic tool the book develops: chaining and Dudley's inequality (Chapter 8), the matrix deviation inequality (Chapter 9), and Gaussian width and the stable dimension (Chapter 7) all combine into a single closing argument.

Setting

Fix a subset T⊆RnT\subseteq\mathbb R^nT⊆Rn. For a standard Gaussian vector g∼N(0,In)g\sim N(0,I_n)g∼N(0,In​), the Gaussian width of TTT is w(T):=Esup⁡x∈T⟨g,x⟩w(T) := \mathbb E\sup_{x\in T}\langle g,x\ranglew(T):=Esupx∈T​⟨g,x⟩ (Chapter 7), and the stable dimension of a bounded TTT is d(T):=w(T)2/diam(T)2d(T) := w(T)^2/\mathrm{diam}(T)^2d(T):=w(T)2/diam(T)2 up to an absolute constant factor (Definition 7.6.2) — a robust substitute for the ordinary linear-algebraic dimension of TTT, which can jump discontinuously under a small perturbation of TTT, unlike d(T)d(T)d(T).

An m×nm\times nm×n Gaussian random matrix with i.i.d. N(0,1)N(0,1)N(0,1) entries is a random matrix AAA each of whose mnmnmn entries is an independent standard normal random variable.

Formalization targets

Goal (Theorem 11.3.3, Dvoretzky-Milman's theorem, Gaussian form)

∃ c>0:m≤cε2d(T)  ⟹  P[(1−ε)B⊆conv(AT)⊆(1+ε)B]≥0.99\exists\,c>0:\quad m\le c\varepsilon^2 d(T) \;\Longrightarrow\; \mathbb P\bigl[(1-\varepsilon)B \subseteq \mathrm{conv}(AT) \subseteq (1+\varepsilon)B\bigr] \ge 0.99∃c>0:m≤cε2d(T)⟹P[(1−ε)B⊆conv(AT)⊆(1+ε)B]≥0.99

for every m×nm\times nm×n Gaussian random matrix AAA with i.i.d. N(0,1)N(0,1)N(0,1) entries, every bounded T⊆RnT\subseteq\mathbb R^nT⊆Rn containing the origin, and every ε∈(0,1)\varepsilon\in(0,1)ε∈(0,1), where BBB is the Euclidean ball of radius w(T)w(T)w(T) centered at the origin. The probability 0.990.990.99 is the book's own literal numeral, not a free parameter — this is the theorem the book actually states, not a family of theorems indexed by a confidence level.

Significance

Dvoretzky-Milman's theorem is one of the foundational results of the local theory of Banach spaces (asymptotic geometric analysis): it says every nnn-dimensional normed space contains an almost-Euclidean subspace of dimension proportional to (a geometric invariant closely related to) log⁡n\log nlogn in the worst case, and much larger for spaces whose unit ball is already well-behaved (the stable dimension of the cube [−1,1]n[-1,1]^n[−1,1]n, for instance, is proportional to nnn itself — Example 11.3.6). This underlies results throughout convex geometry, compressed sensing, and high-dimensional statistics wherever a random low-dimensional projection needs to be shown to preserve geometric structure. The book's own framing makes clear why this chapter is placed last: the theorem's proof is a genuine capstone, invoking Chevet's inequality (itself built from the matrix deviation inequality of Chapter 9, which is built from chaining, Chapter 8) as its main technical tool.

The theorem and its proof are classical (Milman 1971; this book's specific route via Chevet's inequality is a standard modern exposition). This mission formalizes the goal theorem's statement — including its two supporting geometric quantities, Gaussian width and stable dimension, and the notion of a Gaussian random matrix — as a complete, faithful target for a solver, in the book's own sub-namespace built for this chapter (no dependency here is reusable from an earlier chunk, since none of this book series' Chapter 7 or Chapter 9 definitions has yet been published).

Difficulty

The natural first idea — bound conv(AT)\mathrm{conv}(AT)conv(AT) directly using concentration of ∥Ax∥2\|Ax\|_2∥Ax∥2​ for each fixed x∈Tx\in Tx∈T — runs into exactly the uniform-supremum obstacle the whole book has been building tools to overcome: a bound that holds for one xxx at a time, even with a union bound over a net of TTT, does not obviously extend to the full convex hull without first controlling sup⁡x∈T∣⟨Ax,y⟩−w(T)∥y∥2∣\sup_{x\in T}|\langle Ax,y\rangle - w(T)\|y\|_2|supx∈T​∣⟨Ax,y⟩−w(T)∥y∥2​∣ uniformly over both x∈Tx\in Tx∈T and yyy on the unit sphere of the target space — a two-parameter supremum. The book's actual route goes through Chevet's inequality, itself proved using the matrix deviation inequality's own chaining-based argument, to control this two-sided supremum, and then converts the resulting inequality into the containment (1−ε)B⊆conv(AT)⊆(1+ε)B(1-\varepsilon)B\subseteq\mathrm{conv}(AT)\subseteq(1+\varepsilon)B(1−ε)B⊆conv(AT)⊆(1+ε)B via a support- function duality argument (a convex body is pinned down by its support function, so bounding sup⁡x∈T⟨Ax,y⟩\sup_{x\in T}\langle Ax,y\ranglesupx∈T​⟨Ax,y⟩ uniformly over yyy on the sphere is exactly what is needed).

Formalization scope

A is Ω → Matrix (Fin m) (Fin n) ℝ with an explicit IsGaussianMatrix hypothesis (entries i.i.d. N(0,1)N(0,1)N(0,1), formalized entrywise with joint independence). conv(AT) is convexHull ℝ of the image of T under A's mulVec, round-tripped through EuclideanSpace's continuous linear equivalence with the underlying function type. w(T) reuses this mission series' ExpSup/GaussianWidth convention (redefined locally, per the drafts-cannot-import-drafts rule, following the same ProbabilityTheory.stdGaussian-based realization of a standard Gaussian vector as 08-matrix-deviation). The stable dimension d(T)d(T)d(T) is formalized directly as w(T)2/diam(T)2w(T)^2/ \mathrm{diam}(T)^2w(T)2/diam(T)2 rather than via the book's literal (but only asymptotically equivalent, per Exercise 7.6.1) definition through a squared Gaussian width h(T−T)2h(T-T)^2h(T−T)2 — the goal theorem's own proof uses only the inequality direction of that equivalence, and the goal's hypothesis already carries an unpinned absolute constant that absorbs the equivalence constant, so this substitution preserves the theorem's exact truth content (see StableDimension's own doc-comment and MODERATION_NOTES.md for the full argument) rather than approximating it.

Ball-center deviation, disclosed. The book's printed theorem statement carries no hypothesis that TTT contains the origin; its proof opens by translating TTT so that it does ("Translating TTT if necessary, we can assume that TTT contains the origin"), and Remark 11.3.4 then confirms the ball is centered at the origin in that case. This mission states the WLOG-reduced case directly — adding 0∈T0\in T0∈T as an explicit hypothesis — rather than also formalizing the translation argument that recovers the fully general (untranslated) statement. This is disclosed as a genuine narrowing of the literal printed statement, though not of what the book's own proof actually establishes.

This mission covers Theorem 11.3.3 only, with no milestones: BRIEF.md explicitly instructs that if the chapter's full proof chain (general matrix deviation inequality, Chevet's inequality, random projections of sets — Theorems 11.1.5, 11.2.4, 11.3.1) proves too heavy for the session, milestones should be cut rather than the goal substituted. All three are left out, not approximated, given this chapter's five from-scratch definitions already needed for the goal's own statement. ExpSup, GaussianWidth, StableDimension and IsGaussianMatrix are reusable by any later development needing Gaussian width, the stable dimension, or a Gaussian random matrix. Solvers' contributions are welcome on the goal theorem itself and, beyond this mission's current scope, on the three named milestones.

Selected references

  • A. Dvoretzky, Some results on convex bodies and Banach spaces, Proc. Internat. Sympos. Linear Spaces (Jerusalem, 1960), 123–160.
  • V. D. Milman, A new proof of A. Dvoretzky's theorem on cross-sections of convex bodies, Funkcional. Anal. i Priložen. 5 (1971), 28–37.
  • R. Vershynin, High-Dimensional Probability: An Introduction with Applications in Data Science, Cambridge University Press, 2018, Chapter 11. https://doi.org/10.1017/9781108231596
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Machine LearningProbabilityStatistics·Captain: mikedeng1

High-Dimensional Statistics VIII: Oracle Inequalities for Decomposable RegularizersTextbook

Motivation

Chapters 2 through 8 of Wainwright's High-Dimensional Statistics build up sharp error bounds for a sequence of specific high-dimensional models — sparse linear regression via the Lasso (Chapter 7), sparse principal components (Chapter 8) — each proved from scratch with techniques tailored to that model's own penalty and loss. Chapter 9 steps back and asks what made all of those arguments work, and isolates the answer into two structural ingredients: a decomposable regularizer, whose triangle inequality is tight across a well-chosen subspace pair, and a restricted curvature condition on the loss, holding only on the cone that decomposability forces the estimation error into. Once these two ingredients are checked for a particular model, a single, already-proved oracle inequality hands back the error bound — no further optimization-theoretic argument is needed. This mission formalizes that oracle inequality itself, together with its two supporting theorems, as the reusable core the book's later chapters (nuclear-norm matrix regression in Chapter 10, graphical model selection in Chapter 11, group-sparse and overlap-group Lassos) each specialize.

Setting

Let Ω\OmegaΩ be a finite-dimensional real inner product space (e.g. Rd\mathbb R^dRd, or a matrix space with the Frobenius inner product), and consider the regularized M-estimator

θ^∈arg min⁡θ∈Ω{Ln(θ)+λnΦ(θ)},\hat\theta \in \operatorname*{arg\,min}_{\theta\in\Omega} \Big\{ L_n(\theta) + \lambda_n\Phi(\theta) \Big\},θ^∈θ∈Ωargmin​{Ln​(θ)+λn​Φ(θ)},

where Ln:Ω→RL_n:\Omega\to\mathbb RLn​:Ω→R is a convex empirical cost function, Φ:Ω→[0,∞)\Phi:\Omega\to[0,\infty)Φ:Ω→[0,∞) is a norm-based regularizer, and λn>0\lambda_n>0λn​>0 is a user-chosen regularization weight. Write θ∗\theta^*θ∗ for the true parameter and Δ:=θ^−θ∗\Delta:=\hat\theta-\theta^*Δ:=θ^−θ∗ for the estimation error.

A pair of subspaces M⊆Mˉ\mathcal M\subseteq\bar{\mathcal M}M⊆Mˉ of Ω\OmegaΩ — the model subspace and its (possibly larger) closure — has an associated perturbation subspace Mˉ⊥\bar{\mathcal M}^\perpMˉ⊥, the orthogonal complement of Mˉ\bar{\mathcal M}Mˉ. The regularizer Φ\PhiΦ is decomposable with respect to (M,Mˉ)(\mathcal M,\bar{\mathcal M})(M,Mˉ) if the triangle inequality Φ(α+β)≤Φ(α)+Φ(β)\Phi(\alpha+\beta)\le\Phi(\alpha)+\Phi(\beta)Φ(α+β)≤Φ(α)+Φ(β) is an equality whenever α∈M\alpha\in\mathcal Mα∈M and β∈Mˉ⊥\beta\in\bar{\mathcal M}^\perpβ∈Mˉ⊥ — the regularizer penalizes deviations away from the model subspace exactly as much as it possibly could. The canonical example is the ℓ1\ell_1ℓ1​-norm with M=Mˉ\mathcal M=\bar{\mathcal M}M=Mˉ the subspace of vectors supported on a fixed index set SSS.

Writing Φ∗(v):=sup⁡Φ(u)≤1⟨u,v⟩\Phi^*(v):=\sup_{\Phi(u)\le 1}\langle u,v\rangleΦ∗(v):=supΦ(u)≤1​⟨u,v⟩ for the dual norm, the good event G(λn):={Φ∗(∇Ln(θ∗))≤λn/2}\mathcal G(\lambda_n):=\{\Phi^*(\nabla L_n(\theta^*))\le\lambda_n/2\}G(λn​):={Φ∗(∇Ln​(θ∗))≤λn​/2} says the regularization weight dominates the dual norm of the score function at the truth — the non-probabilistic conditioning hypothesis every result in this chapter is stated under. The subspace Lipschitz constant Ψ(S):=sup⁡u∈S∖{0}Φ(u)/∥u∥\Psi(S):=\sup_{u\in S\setminus\{0\}}\Phi(u)/\|u\|Ψ(S):=supu∈S∖{0}​Φ(u)/∥u∥ measures the worst-case price of converting between the regularizer Φ\PhiΦ and the error norm ∥⋅∥\|\cdot\|∥⋅∥ on a subspace SSS.

Formalization targets

Goal (Theorem 9.19, "Bounds for general models")

Under (A1) LnL_nLn​ convex, satisfying restricted strong convexity (RSC) with curvature κ>0\kappa>0κ>0, radius RRR and tolerance τn2\tau_n^2τn2​ — En(Δ):=Ln(θ∗+Δ)−Ln(θ∗)−⟨∇Ln(θ∗),Δ⟩≥κ2∥Δ∥2−τn2Φ2(Δ)E_n(\Delta):=L_n(\theta^*+\Delta)-L_n(\theta^*) -\langle\nabla L_n(\theta^*),\Delta\rangle \ge \frac{\kappa}{2}\|\Delta\|^2-\tau_n^2\Phi^2(\Delta)En​(Δ):=Ln​(θ∗+Δ)−Ln​(θ∗)−⟨∇Ln​(θ∗),Δ⟩≥2κ​∥Δ∥2−τn2​Φ2(Δ) for ∥Δ∥≤R\|\Delta\|\le R∥Δ∥≤R — and (A2) Φ\PhiΦ decomposable with respect to (M,Mˉ)(\mathcal M,\bar{\mathcal M})(M,Mˉ): conditioned on G(λn)\mathcal G(\lambda_n)G(λn​), any optimal θ^\hat\thetaθ^ satisfies

(a)Φ(θ^−θ∗)≤4(Ψ(Mˉ) ∥θ^−θ∗∥+Φ(θM⊥∗)),\text{(a)}\quad \Phi(\hat\theta-\theta^*) \le 4\big(\Psi(\bar{\mathcal M})\, \|\hat\theta-\theta^*\| + \Phi(\theta^*_{\mathcal M^\perp})\big),(a)Φ(θ^−θ∗)≤4(Ψ(Mˉ)∥θ^−θ∗∥+Φ(θM⊥∗​)),

and, whenever τn2Ψ2(Mˉ)≤κ/64\tau_n^2\Psi^2(\bar{\mathcal M})\le\kappa/64τn2​Ψ2(Mˉ)≤κ/64 and εn(M,Mˉ)≤R\varepsilon_n(\mathcal M,\bar{\mathcal M})\le Rεn​(M,Mˉ)≤R,

(b)∥θ^−θ∗∥2≤εn2(M,Mˉ):=9λn2κ2Ψ2(Mˉ)+8κ(λnΦ(θM⊥∗)+16τn2Φ2(θM⊥∗)).\text{(b)}\quad \|\hat\theta-\theta^*\|^2 \le \varepsilon_n^2(\mathcal M,\bar{\mathcal M}) := \frac{9\lambda_n^2}{\kappa^2}\Psi^2(\bar{\mathcal M}) + \frac{8}{\kappa}\Big(\lambda_n\Phi(\theta^*_{\mathcal M^\perp}) + 16\tau_n^2\Phi^2(\theta^*_{\mathcal M^\perp})\Big).(b)∥θ^−θ∗∥2≤εn2​(M,Mˉ):=κ29λn2​​Ψ2(Mˉ)+κ8​(λn​Φ(θM⊥∗​)+16τn2​Φ2(θM⊥∗​)).

Milestones

  • Proposition 9.13. Under (A2) alone, conditioned on G(λn)\mathcal G(\lambda_n)G(λn​), the error Δ=θ^−θ∗\Delta=\hat\theta-\theta^*Δ=θ^−θ∗ lies in the cone Cθ∗(M,Mˉ):={Δ∣Φ(ΔMˉ⊥)≤3Φ(ΔMˉ)+4Φ(θM⊥∗)}\mathbb C_{\theta^*}(\mathcal M,\bar{\mathcal M}):=\{\Delta\mid\Phi(\Delta_{\bar{\mathcal M}^\perp})\le 3\Phi(\Delta_{\bar{\mathcal M}})+4\Phi(\theta^*_{\mathcal M^\perp})\}Cθ∗​(M,Mˉ):={Δ∣Φ(ΔMˉ⊥​)≤3Φ(ΔMˉ​)+4Φ(θM⊥∗​)} — the purely geometric fact Theorem 9.19's curvature argument is built on.
  • Corollary 9.20. When θ∗∈M\theta^*\in\mathcal Mθ∗∈M exactly, the approximation-error term of εn2\varepsilon_n^2εn2​ vanishes and Theorem 9.19 collapses to Φ(θ^−θ∗)≤6λnκΨ2(Mˉ)\Phi(\hat\theta-\theta^*)\le\frac{6\lambda_n}{\kappa}\Psi^2(\bar{\mathcal M})Φ(θ^−θ∗)≤κ6λn​​Ψ2(Mˉ), ∥θ^−θ∗∥2≤9λn2κ2Ψ2(Mˉ)\|\hat\theta-\theta^*\|^2\le\frac{9\lambda_n^2}{\kappa^2}\Psi^2(\bar{\mathcal M})∥θ^−θ∗∥2≤κ29λn2​​Ψ2(Mˉ) — the form used directly against every concrete model in the rest of the book.
  • Theorem 9.24. Under an alternative, gradient-based curvature condition (Φ∗\Phi^*Φ∗-curvature, Definition 9.22) and θ∗∈M\theta^*\in\mathcal Mθ∗∈M, the dual-norm error is controlled directly: Φ∗(θ^−θ∗)≤3λn/κ\Phi^*(\hat\theta-\theta^*)\le 3\lambda_n/\kappaΦ∗(θ^−θ∗)≤3λn​/κ.

Significance

Theorem 9.19 is the book's own claimed unifying result: as it remarks explicitly, the theorem is a deterministic implication, and every later probabilistic corollary in Parts II and III of the book is obtained by (i) checking that a specific loss/regularizer pair is decomposable with respect to a natural subspace pair for the problem at hand, (ii) certifying the RSC condition with high probability for that loss (via concentration arguments from Chapters 2–6), and (iii) choosing λn\lambda_nλn​ large enough that the good event holds with high probability — then reading off the rate directly from εn2(M,Mˉ)\varepsilon_n^2(\mathcal M,\bar{\mathcal M})εn2​(M,Mˉ). Chapter 7's Lasso bound (Theorem 7.13, mission 07-sparse-linear) is exactly Corollary 9.20 specialized to Φ=∥⋅∥1\Phi=\|\cdot\|_1Φ=∥⋅∥1​ and M\mathcal MM the subspace of sss-sparse vectors — but Chapter 9 proves it once, in a form that Chapter 10's nuclear-norm-regularized low-rank matrix regression (mission 10-matrix-rank), Chapter 11's graphical model selection, and the chapter's own group-Lasso and overlap-group-Lasso examples all instantiate without re-deriving the optimization argument.

Difficulty

The formalization difficulty here is almost entirely conceptual rather than syntactic: getting the two-subspace apparatus (M,Mˉ)(\mathcal M,\bar{\mathcal M})(M,Mˉ) exactly right. The book explicitly allows Mˉ\bar{\mathcal M}Mˉ to be a strict superset of M\mathcal MM (needed for the nuclear norm in Chapter 10, where the naive choice M=Mˉ\mathcal M=\bar{\mathcal M}M=Mˉ fails to be decomposable at all), so every definition and theorem in this mission is parameterized by the pair, not by a single subspace — and three genuinely different projections appear across the statements: the error vector's projection onto Mˉ\bar{\mathcal M}Mˉ and onto Mˉ⊥\bar{\mathcal M}^\perpMˉ⊥ (both keep the bar), versus the true parameter's projection onto M⊥\mathcal M^\perpM⊥ (the complement of the small, unbarred subspace). A further subtlety specific to this printed source: several of the book's own displayed equations for Ψ(⋅)\Psi(\cdot)Ψ(⋅) in Theorem 9.19 and Corollary 9.20 lose the overbar on Mˉ\bar{\mathcal M}Mˉ in PDF text extraction (a rendering artifact, not a mathematical ambiguity); resolving which subspace is meant required reading the surrounding proof text line by line, since only Ψ(Mˉ)\Psi(\bar{\mathcal M})Ψ(Mˉ) — not Ψ(M)\Psi(\mathcal M)Ψ(M) — is mathematically consistent with how the constant is derived and used (see MODERATION_NOTES.md).

Formalization scope

Ω\OmegaΩ is [NormedAddCommGroup Ω] [InnerProductSpace ℝ Ω] [FiniteDimensional ℝ Ω], matching the book's implicit assumption of a finite-dimensional inner-product parameter space throughout this part of the book. The regularizer's norm axioms (IsRegularizerNorm), the dual norm, and the subspace Lipschitz constant are all defined via sSup/sInf-free explicit formulas or sSup over an explicitly-described set (never an unconstrained supremum over all of Ω\OmegaΩ), so no faithfulness trap from an unbounded or empty supremum arises (see MODERATION_NOTES.md's trap table). κ > 0 and λ_n > 0 are made explicit hypotheses of every theorem, matching Definition 9.15's own stated positivity of κ\kappaκ and the chapter's running convention that λn\lambda_nλn​ is a positive regularization weight — never a narrowing of the theorem's actual scope. A trivializing formalization of this chapter would either collapse the two-subspace machinery to a single subspace M=Mˉ\mathcal M=\bar{\mathcal M}M=Mˉ (which is faithful only for the ℓ1\ell_1ℓ1​/group-Lasso examples, not the general theorem, and not what Chapter 10 needs) or silently drop the second conjunct of Theorem 9.19's conclusion (part (b), the actual quantitative rate) in favor of only the qualitative part (a); this mission formalizes the full two-subspace statement and both conjuncts of the goal theorem. Out of scope: the chapter's worked examples (sparse GLMs, Corollary 9.26; group Lasso; nuclear-norm matrix regression) that specialize the goal to concrete models — Chapter 10's own mission (10-matrix-rank) restates the needed instance of this framework locally rather than importing this mission's draft, per this book's series-wide convention that no draft imports another chunk's draft. Also out of scope: the RSC-implies-restricted-eigenvalue correspondence (Example 9.16) and the μn(Φ∗)\mu_n(\Phi^*)μn​(Φ∗)-based general RSC certification (Theorem 9.36, Section 9.8), both purely probabilistic results that lie outside this chapter's own deterministic core.

Selected references

  • Wainwright, M. J. High-Dimensional Statistics: A Non-Asymptotic Viewpoint. Cambridge University Press, 2019. Chapter 9. DOI: 10.1017/9781108627771.
  • Negahban, S. N., Ravikumar, P., Wainwright, M. J., Yu, B. "A unified framework for high-dimensional analysis of M-estimators with decomposable regularizers." Statistical Science, 27(4), 2012, 538–557.
  • Tibshirani, R. "Regression shrinkage and selection via the Lasso." Journal of the Royal Statistical Society: Series B, 58(1), 1996, 267–288.
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Machine LearningProbabilityStatistics·Captain: mikedeng1

High-Dimensional Statistics IX: Nuclear-Norm Regularization for Low-Rank Matrix RegressionTextbook

Motivation

Many estimation problems are naturally posed over matrices rather than vectors: recommender systems (Netflix-style matrix completion), multivariate regression with correlated responses, vector autoregressive time series, and phase retrieval all reduce to estimating an unknown matrix Θ∗\Theta^*Θ∗ that is low-rank, or well approximated by one. A rank constraint alone makes the natural least-squares estimator non-convex and generally intractable; replacing it with the nuclear norm — the sum of the matrix's singular values, the tightest convex surrogate for rank — yields a tractable semidefinite program. Wainwright's High-Dimensional Statistics (2019), Chapter 10, shows that this substitution costs nothing statistically: nuclear-norm-regularized least squares achieves error rates matching what one could hope for even knowing the rank in advance, by specializing Chapter 9's general decomposable-regularizer framework (mission 09-decomposability) directly to the nuclear norm.

Setting

For matrices A,B∈Rd1×d2A,B\in\mathbb R^{d_1\times d_2}A,B∈Rd1​×d2​, the trace inner product is ⟨ ⁣⟨A,B⟩ ⁣⟩:=trace(ATB)=∑j1,j2Aj1j2Bj1j2\langle\!\langle A,B\rangle\!\rangle := \mathrm{trace}(A^TB) = \sum_{j_1,j_2}A_{j_1j_2}B_{j_1j_2}⟨⟨A,B⟩⟩:=trace(ATB)=∑j1​,j2​​Aj1​j2​​Bj1​j2​​ (Eq. 10.1), inducing the Frobenius norm ∥ ⁣∣A∣ ⁣∥F\|\!|A|\!\|_F∥∣A∣∥F​. Given design matrices X1,…,Xn∈Rd1×d2X_1,\dots,X_n\in\mathbb R^{d_1\times d_2}X1​,…,Xn​∈Rd1​×d2​ and responses yi=⟨ ⁣⟨Xi,Θ∗⟩ ⁣⟩+wiy_i=\langle\!\langle X_i,\Theta^*\rangle\!\rangle+w_iyi​=⟨⟨Xi​,Θ∗⟩⟩+wi​, the observation operator Xn(Θ):=(⟨ ⁣⟨Xi,Θ⟩ ⁣⟩)i=1n\mathcal X_n(\Theta):=(\langle\!\langle X_i,\Theta\rangle\!\rangle)_{i=1}^nXn​(Θ):=(⟨⟨Xi​,Θ⟩⟩)i=1n​ and its adjoint Xn∗(u):=∑iuiXi\mathcal X_n^*(u):=\sum_iu_iX_iXn∗​(u):=∑i​ui​Xi​ (Eqs. 10.2-10.3) are the matrix analogs of a vector design matrix and its transpose. The nuclear norm ∥ ⁣∣Θ∣ ⁣∥nuc:=∑jσj(Θ)\|\!|\Theta|\!\|_{\mathrm{nuc}}:=\sum_j\sigma_j(\Theta)∥∣Θ∣∥nuc​:=∑j​σj​(Θ) (Eq. 10.5) — the sum of singular values — is a decomposable regularizer (in the sense of Chapter 9) with respect to the subspace pair spanned by the top singular vectors of any target matrix, and its dual norm (Table 9.1) is the ℓ2\ell_2ℓ2​-operator (spectral) norm ∥ ⁣∣⋅∣ ⁣∥2\|\!|\cdot|\!\|_2∥∣⋅∣∥2​. The estimator under study is nuclear-norm-regularized least squares,

Θ^∈arg min⁡Θ∈Rd1×d2{12n∥y−Xn(Θ)∥22+λn∥ ⁣∣Θ∣ ⁣∥nuc}(10.16)\hat\Theta \in \operatorname*{arg\,min}_{\Theta\in\mathbb R^{d_1\times d_2}} \left\{ \frac{1}{2n}\|y-\mathcal X_n(\Theta)\|_2^2 + \lambda_n\|\!|\Theta|\!\|_{\mathrm{nuc}} \right\} \tag{10.16}Θ^∈Θ∈Rd1​×d2​argmin​{2n1​∥y−Xn​(Θ)∥22​+λn​∥∣Θ∣∥nuc​}(10.16)

with λn>0\lambda_n>0λn​>0 user-chosen.

Formalization targets

Goal (Proposition 10.6)

Suppose Xn\mathcal X_nXn​ satisfies the restricted strong convexity condition (10.17), ∥Xn(Δ)∥22/(2n)≥κ/2∥ ⁣∣Δ∣ ⁣∥F2−c0d1+d2n∥ ⁣∣Δ∣ ⁣∥nuc2\|\mathcal X_n(\Delta)\|_2^2/(2n) \ge \kappa/2\|\!|\Delta|\!\|_F^2 - c_0\frac{d_1+d_2}{n}\|\!|\Delta|\!\|_{\mathrm{nuc}}^2∥Xn​(Δ)∥22​/(2n)≥κ/2∥∣Δ∣∥F2​−c0​nd1​+d2​​∥∣Δ∣∥nuc2​ for all Δ\DeltaΔ, with κ>0\kappa>0κ>0, c0≥0c_0\ge 0c0​≥0. Conditioned on the good event G(λn)={∥ ⁣∣1n∑iwiXi∣ ⁣∥2≤λn/2}\mathcal G(\lambda_n)=\{\|\!|\frac1n\sum_iw_iX_i|\!\|_2 \le\lambda_n/2\}G(λn​)={∥∣n1​∑i​wi​Xi​∣∥2​≤λn​/2}, any optimal Θ^\hat\ThetaΘ^ satisfies, for any r∈{1,…,d′}r\in\{1,\dots,d'\}r∈{1,…,d′} with r≤κn/(128c0(d1+d2))r\le\kappa n/(128c_0(d_1+d_2))r≤κn/(128c0​(d1​+d2​)),

∥ ⁣∣Θ^−Θ∗∣ ⁣∥F2≤92λn2κ2r+1κ{2λn∑j=r+1d′σj(Θ∗)+32c0(d1+d2)n(∑j=r+1d′σj(Θ∗))2}.\|\!|\hat\Theta-\Theta^*|\!\|_F^2 \le \frac{9}{2}\frac{\lambda_n^2}{\kappa^2}r + \frac{1}{\kappa}\left\{2\lambda_n\sum_{j=r+1}^{d'}\sigma_j(\Theta^*) + \frac{32c_0(d_1+d_2)}{n}\left(\sum_{j=r+1}^{d'}\sigma_j(\Theta^*)\right)^2\right\}.∥∣Θ^−Θ∗∣∥F2​≤29​κ2λn2​​r+κ1​⎩⎨⎧​2λn​j=r+1∑d′​σj​(Θ∗)+n32c0​(d1​+d2​)​​j=r+1∑d′​σj​(Θ∗)​2⎭⎬⎫​.

Milestone (Proposition 10.7)

Under the alternative Φ∗\Phi^*Φ∗-curvature condition (10.20) (a curvature bound on the gradient map rather than the Taylor error), with rank(Θ∗)<κ/(64τn)\mathrm{rank}(\Theta^*)<\kappa/(64\tau_n)rank(Θ∗)<κ/(64τn​): conditioned on G(λn)={∥ ⁣∣1nXn∗(w)∣ ⁣∥2≤λn/2}\mathcal G(\lambda_n)=\{\|\!|\frac1n\mathcal X_n^*(w)|\!\|_2\le\lambda_n/2\}G(λn​)={∥∣n1​Xn∗​(w)∣∥2​≤λn​/2}, any optimal Θ^\hat\ThetaΘ^ satisfies ∥ ⁣∣Θ^−Θ∗∣ ⁣∥2≤32 λn/κ\|\!|\hat\Theta-\Theta^*|\!\|_2 \le 3\sqrt2\,\lambda_n/\kappa∥∣Θ^−Θ∗∣∥2​≤32​λn​/κ — an operator-norm bound the book notes is, in conjunction with the cone-like constraint (10.15), strictly stronger than Proposition 10.6's Frobenius-norm bound.

Significance

Proposition 10.6 is this chapter's direct payoff from Chapter 9's general machinery: it shows that the deterministic backbone of the Lasso's guarantee (mission 07-sparse-linear) extends essentially verbatim to the matrix setting, with the sparsity level sss replaced by the target rank rrr and the ambient dimension ddd replaced by d1+d2d_1+d_2d1​+d2​ — exactly the "degrees of freedom" scaling one would predict by counting the parameters needed to specify a rank-rrr matrix. Every one of the chapter's later corollaries (matrix compressed sensing, multivariate regression, matrix completion) is obtained by verifying the restricted strong convexity condition (10.17) holds with high probability for a specific random design, then reading the rate directly off Proposition 10.6 — the same two-step recipe Chapter 9's own Theorem 9.19 established abstractly. Proposition 10.7's operator-norm bound is what subsequently controls the individual singular values of the estimation error, needed for exact-rank-recovery guarantees.

Difficulty

Both results are direct specializations of Chapter 9's general oracle inequalities (Theorem 9.19 and Theorem 9.24 respectively) to the nuclear norm as regularizer and the Frobenius/operator norm pair, so their formalization difficulty lies almost entirely in getting the matrix-specific objects right rather than in new proof machinery: the nuclear norm requires an actual notion of singular values (realized via the eigenvalues of the Gram matrix ΘTΘ\Theta^T\ThetaΘTΘ, using Mathlib's Hermitian-matrix spectral theorem), the operator norm requires the correct rectangular generalization of the symmetric-matrix Rayleigh-quotient characterization used in mission 08-pca, and the restricted-strong-convexity and curvature conditions must be instantiated against the correctly-adjointed observation operator Xn∗\mathcal X_n^*Xn∗​. A further subtlety is keeping Proposition 10.6's Frobenius-norm conclusion and Proposition 10.7's operator-norm conclusion cleanly distinct — the book itself warns against conflating the norms used across different chapters of Part II (the vector ℓ2\ell_2ℓ2​-norm of chunks 07-sparse-linear/08-pca versus the matrix Frobenius and operator norms here).

Formalization scope

Scope cut, disclosed here and in STATUS.md. BRIEF.md recommends Corollary 10.10 (the sample-complexity bound for the Σ\SigmaΣ-Gaussian random matrix ensemble) as the goal theorem. Corollary 10.10 is a genuinely probabilistic statement — it asserts a bound holding "with probability at least 1−2e−2nδ21-2e^{-2n\delta^2}1−2e−2nδ2" over nnn i.i.d. draws of design matrices from a Σ\SigmaΣ-Gaussian ensemble (Theorem 10.8's own high-probability restricted-strong-convexity certification for that ensemble) — and formalizing it faithfully would require a genuine multivariate-Gaussian-measure infrastructure on matrix space (a probability space, an i.i.d. sequence of Σ\SigmaΣ-covariance-structured Gaussian matrices, and Mathlib's measure-theoretic probability API) that is disproportionate to this mission's time budget, and orthogonal to what Chapter 10 itself contributes (the chapter's own text stresses that Propositions 10.6 and 10.7 are the chapter's deterministic core, with probability entering only in Section 10.3's ensemble-specific certification — precisely mirroring chunk 09-decomposability's own "Theorem 9.19 is actually a deterministic result" framing). This mission instead takes Proposition 10.6 as its goal — explicitly named in BRIEF.md's own candidate list as "the nuclear-norm oracle inequality, an explicit corollary of Theorem 9.19" — the natural, tractable, still highly citable deterministic title result of Section 10.2, together with its companion Proposition 10.7. Theorem 10.8 (the Σ\SigmaΣ-Gaussian ensemble's RSC certification), Corollary 10.9 (noiseless exact recovery) and Corollary 10.10 itself are left for a future mission with a dedicated probability-theory budget. The cone-like constraint (Eq. 10.15) — whose own faithful statement requires the same explicit subspace-pair machinery (M(Ur,Vr),Mˉ(Ur,Vr)\mathcal M(U_r,V_r),\bar{\mathcal M}(U_r,V_r)M(Ur​,Vr​),Mˉ(Ur​,Vr​)) chunk 09-decomposability built for the general theory — is similarly left out, since Propositions 10.6 and 10.7's own numbered statements never expose these subspaces directly (only their proofs do, via instantiating Theorem 9.19/9.24). singularValues and nuclearNorm are noncomputable, defined via Mathlib's Hermitian-matrix eigenvalue spectral theorem; c0 ≥ 0 and λn > 0 are made explicit, matching this book's running conventions for RSC tolerance constants and regularization weights (see MODERATION_NOTES.md).

Selected references

  • Wainwright, M. J. High-Dimensional Statistics: A Non-Asymptotic Viewpoint. Cambridge University Press, 2019. Chapter 10. DOI: 10.1017/9781108627771.
  • Negahban, S., Wainwright, M. J. "Estimation of (near) low-rank matrices with noise and high-dimensional scaling." Annals of Statistics, 39(2), 2011, 1069–1097.
  • Recht, B., Fazel, M., Parrilo, P. A. "Guaranteed minimum-rank solutions of linear matrix equations via nuclear norm minimization." SIAM Review, 52(3), 2010, 471–501.
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Machine LearningProbabilityStatistics·Captain: mikedeng1

High-Dimensional Statistics X: Graph Selection Consistency for Gaussian Graphical ModelsTextbook

Motivation

Many high-dimensional data sets — gene-expression profiles, sensor networks, social interactions — come with no natural ordering of variables, only pairwise dependencies whose structure is itself the object of interest. A graphical model encodes these dependencies as an undirected graph: vertices are variables, and edges mark direct (conditional) dependence. Recovering the graph from samples — graphical model selection — is a combinatorial problem masquerading as a statistical one: there are 2(d2)2^{\binom{d}{2}}2(2d​) candidate graphs on ddd vertices, far too many to search directly. For Gaussian data, however, graph structure is exactly the sparsity pattern of the inverse covariance (precision) matrix, which turns graph selection into ddd coupled sparse-regression problems — one per vertex — each of which the Lasso theory of Chapter 7 already knows how to solve. This mission formalizes the theorem, due to Meinshausen and Bühlmann (2006), that shows this reduction actually works: solving ddd independent Lasso problems and combining the results recovers the exact graph with high probability, at a sample complexity governed by the same kind of incoherence condition that governs Lasso support recovery itself.

Setting

An undirected graphical model on a finite vertex set VVV pairs a graph G=(V,E)G=(V,E)G=(V,E) with a random vector X=(Xj)j∈VX=(X_j)_{j\in V}X=(Xj​)j∈V​. Two equivalent structural properties connect XXX to GGG (Theorem 11.8, Hammersley-Clifford): XXX factorizes according to GGG if its density is a product of nonnegative functions, one per clique of GGG, each depending only on the variables in that clique (Definition 11.1); XXX is Markov with respect to GGG if, for every vertex cutset SSS separating VVV into disjoint pieces AAA and BBB, the sub-vectors XAX_AXA​ and XBX_BXB​ are conditionally independent given XSX_SXS​ (Definition 11.5). For a strictly positive density, these are the same condition.

For a zero-mean ddd-dimensional Gaussian vector with covariance Σ∗\Sigma^*Σ∗ and precision matrix Θ∗=(Σ∗)−1\Theta^*=(\Sigma^*)^{-1}Θ∗=(Σ∗)−1, the graph structure is exactly the support of Θ∗\Theta^*Θ∗: (j,k)∈E  ⟺  Θjk∗≠0(j,k)\in E \iff \Theta^*_{jk}\ne0(j,k)∈E⟺Θjk∗​=0. The neighborhood N(j):={k∣(j,k)∈E}N(j):=\{k\mid(j,k)\in E\}N(j):={k∣(j,k)∈E} of each vertex is itself a vertex cutset (separating {j}\{j\}{j} from everything else), so the conditional independence Xj⊥XV∖N+(j)∣XN(j)X_j\perp X_{V\setminus N^+(j)}\mid X_{N(j)}Xj​⊥XV∖N+(j)​∣XN(j)​ holds, and — by standard Gaussian conditioning — XjX_jXj​ decomposes as a linear function of XV∖{j}X_{V\setminus\{j\}}XV∖{j}​ plus independent Gaussian noise, with regression coefficients supported exactly on N(j)N(j)N(j). Neighborhood regression exploits this directly: for each vertex jjj, solve the Lasso

θ^j∈arg⁡min⁡θ∈Rd−1 12n∥Xj−X∖{j}θ∥22+λn∥θ∥1,\hat\theta_j \in \arg\min_{\theta\in\mathbb R^{d-1}}\ \frac1{2n}\|X_j-X_{\setminus\{j\}}\theta\|_2^2 +\lambda_n\|\theta\|_1,θ^j​∈argθ∈Rd−1min​ 2n1​∥Xj​−X∖{j}​θ∥22​+λn​∥θ∥1​,

read off N^(j):={k∣θ^j,k≠0}\hat N(j):=\{k\mid\hat\theta_{j,k}\ne0\}N^(j):={k∣θ^j,k​=0}, and combine the ddd per-vertex estimates into a single edge set via the OR rule ((j,k)∈E^OR(j,k)\in\hat E_{\mathrm{OR}}(j,k)∈E^OR​ iff k∈N^(j)k\in\hat N(j)k∈N^(j) or j∈N^(k)j\in\hat N(k)j∈N^(k)) or the more conservative AND rule (iff both hold). The relevant incoherence condition, analogous to Chapter 7's, is stated for a positive definite matrix Γ\GammaΓ and subset SSS: Γ\GammaΓ is α\alphaα-incoherent with respect to SSS if max⁡k∉S∥ΓkS(ΓSS)−1∥1≤1−α\max_{k\notin S}\|\Gamma_{kS}(\Gamma_{SS})^{-1}\|_1\le1-\alphamaxk∈/S​∥ΓkS​(ΓSS​)−1∥1​≤1−α.

Formalization targets

Theorem 11.8 (Hammersley-Clifford). Factorizes G p ↔ IsMarkov G X P for any strictly positive density ppp.

Theorem 11.12 (goal — graph selection consistency). Suppose for every jjj, Σ∖{j}∗\Sigma^*_{\setminus\{j\}}Σ∖{j}∗​ is α\alphaα-incoherent with respect to N(j)N(j)N(j), and ∣ ⁣∣ ⁣∣(ΣN(j),N(j)∗)−1∣ ⁣∣ ⁣∣∞≤b|\!|\!|(\Sigma^*_{N(j),N(j)})^{-1}|\!|\!|_\infty\le b∣∣∣(ΣN(j),N(j)∗​)−1∣∣∣∞​≤b. With λn=c01α(log⁡d/n+δ)\lambda_n=c_0\frac1\alpha(\sqrt{\log d/n}+\delta)λn​=c0​α1​(logd/n​+δ), the neighborhood-Lasso estimate combined via either rule satisfies, with probability at least 1−c2e−c3nmin⁡(δ2,1/m)1-c_2e^{-c_3n\min(\delta^2,1/m)}1−c2​e−c3​nmin(δ2,1/m):

E^⊆Eand∀(j,k): ∣Θjk∗∣≥7bλn  ⟹  (j,k)∈E^.\hat E\subseteq E \qquad\text{and}\qquad \forall (j,k):\ |\Theta^*_{jk}|\ge7b\lambda_n \implies (j,k)\in\hat E.E^⊆Eand∀(j,k): ∣Θjk∗​∣≥7bλn​⟹(j,k)∈E^.

Significance

Theorem 11.12 is the statistical justification for one of the two standard approaches to Gaussian graphical model selection (the other being the penalized-likelihood "graphical Lasso" of §11.2.1). Its significance is computational as much as statistical: rather than solving one ddd-dimensional penalized-likelihood problem, neighborhood regression solves ddd independent, embarrassingly parallel Lasso problems, each of dimension d−1d-1d−1 — a substantial practical advantage at scale, with (as this theorem shows) no loss in statistical guarantee. Formalizing it produces, for the first time on the platform, statement-level infrastructure for undirected graphical models (Hammersley-Clifford, the Markov property via vertex cutsets, neighborhood structure) together with the random-design analogue of the Lasso support-recovery machinery — a genuinely different technical regime from Chapter 7's fixed-design Lasso theory, since here the "design matrix" X∖{j}X_{\setminus\{j\}}X∖{j}​ is itself Gaussian and statistically coupled to the response XjX_jXj​ through the very covariance structure being estimated. As with the other missions in this series, only the statements are formalized here; the proofs (an extension of the primal-dual witness technique to random design, per the book's own proof sketch) are left as the draft goal for future proof contributions.

Difficulty

The proof of Theorem 7.21 (Chapter 7's Lasso support-recovery guarantee) is for a deterministic design matrix, with all randomness confined to the additive noise. Here the "design" X∖{j}X_{\setminus\{j\}}X∖{j}​ is itself random and Gaussian, and — critically — it is statistically dependent on the very quantity (N(j)N(j)N(j), encoded in Θ∗\Theta^*Θ∗'s support) the Lasso is trying to recover, since X∖{j}X_{\setminus\{j\}}X∖{j}​'s own covariance structure is exactly what the incoherence condition constrains. The naive approach of just conditioning on the realized design matrix and invoking Theorem 7.21 fails, because the deterministic-design incoherence condition would then need to hold for the sample covariance Γ=1nX∖{j}TX∖{j}\Gamma=\frac1n X_{\setminus\{j\}}^TX_{\setminus\{j\}}Γ=n1​X∖{j}T​X∖{j}​, not the population covariance Σ∖{j}∗\Sigma^*_{\setminus\{j\}}Σ∖{j}∗​ that is actually assumed — and controlling the gap between sample and population incoherence under the joint (not fixed) randomness of predictors and response is exactly the extra step the book's proof needs, handled via an extension of the primal-dual witness technique that tracks both sources of randomness together.

Formalization scope

The vertex set V is an arbitrary finite type; the covariate space for X is ℝ throughout (all variables jointly Gaussian). The Gaussian design is characterized via its one-dimensional projections (every linear combination is univariate Gaussian with the matching variance) rather than via Mathlib's multivariate-Gaussian machinery directly, to keep the definition self-contained. IsAlphaIncoherent's ambient index set is realized as a subset of the full vertex type rather than as a literal submatrix, since the book's condition never references an entry outside it. The theorem states the conclusion jointly for both the OR-rule and AND-rule estimated edge sets on one shared high-probability event, matching "based on either rule" literally rather than picking one. The trivializing formalization ruled out here is treating the neighborhood-Lasso estimate as a fixed-design Lasso problem (silently dropping the joint randomness of predictors and response) — every design realization in this formalization is the actual random vector Xdes i ω, not a deterministic parameter, and the Gaussian design hypothesis (IsIIDGaussianDesign) is stated over the same probability space Ω as the least-squares residual. Theorem 11.8 (Hammersley–Clifford) is formalized only for the continuous case — a random vector with a density with respect to Lebesgue measure — matching what the Gaussian goal (Theorem 11.12) actually needs; the book's own Definition 11.1 also permits a discrete (counting-measure) density, with the Ising model (Example 11.4) as a worked instance, which this mission does not cover. Contributions welcome: the graphical Lasso's own guarantees (Propositions 11.9, 11.10, deferred from this mission — see STATUS.md), and the proof of Theorem 11.12 itself via the primal-dual witness extension the book sketches.

Selected references

  • M. Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint, Cambridge University Press, 2019, Chapter 11. https://doi.org/10.1017/9781108627771
  • N. Meinshausen and P. Bühlmann, "High-dimensional graphs and variable selection with the Lasso," Annals of Statistics, 34(3):1436-1462, 2006. https://doi.org/10.1214/009053606000000281
  • J. Hammersley and P. Clifford, "Markov fields on finite graphs and lattices," unpublished manuscript, 1971.
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Functional AnalysisMachine LearningProbability+1·Captain: mikedeng1

High-Dimensional Statistics XI: The Moore-Aronszajn TheoremTextbook

Motivation

Many statistical problems — nonparametric regression, density estimation, dimension reduction, testing — are naturally posed as optimization over a space of functions rather than a finite-dimensional parameter vector. Hilbert spaces provide the right generality: they carry an inner product and a norm, so notions of projection, orthogonality and least-squares fitting all make sense, exactly as in ordinary Euclidean space, even though the "vectors" are now functions. Reproducing kernel Hilbert spaces (RKHSs) are the particular class of function-valued Hilbert spaces that make this program computationally tractable: they are generated by a single bivariate kernel function, and every RKHS computation reduces to evaluating that kernel, never to manipulating an infinite-dimensional object directly (the "kernel trick"). Wainwright's High-Dimensional Statistics (2019), Chapter 12, develops the foundational correspondence between kernels and Hilbert spaces that makes this possible, and this mission formalizes its two central theorems.

Setting

A Hilbert space is a complete inner product space (Definitions 12.1–12.2); this mission uses Mathlib's own NormedAddCommGroup/InnerProductSpace ℝ/CompleteSpace typeclasses for this notion throughout. A linear functional L:H→RL:H\to\mathbb RL:H→R is bounded if ∣L(f)∣≤M∥f∥H|L(f)|\le M\|f\|_H∣L(f)∣≤M∥f∥H​ for some M<∞M<\inftyM<∞ and all f∈Hf\in Hf∈H; the Riesz representation theorem (Theorem 12.5) says every such functional is L(f)=⟨f,g⟩HL(f)=\langle f,g\rangle_HL(f)=⟨f,g⟩H​ for a unique g∈Hg\in Hg∈H.

A bivariate function K:X×X→RK:X\times X\to\mathbb RK:X×X→R is a positive semidefinite (PSD) kernel (Definition 12.6) if it is symmetric and every finite Gram matrix (K(xi,xj))i,j=1n(K(x_i,x_j))_{i,j=1}^n(K(xi​,xj​))i,j=1n​ is positive semidefinite — the natural generalization of a PSD matrix to a (possibly infinite) index set XXX, with no topological structure on XXX required. A reproducing kernel Hilbert space (RKHS) for a kernel KKK is a Hilbert space HHH of functions on XXX such that, for every x∈Xx\in Xx∈X, the function K(⋅,x)K(\cdot,x)K(⋅,x) belongs to HHH and

⟨f,K(⋅,x)⟩H=f(x)for all f∈H(12.3)\langle f, K(\cdot,x)\rangle_H = f(x) \qquad \text{for all } f\in H \tag{12.3}⟨f,K(⋅,x)⟩H​=f(x)for all f∈H(12.3)

— the reproducing property. Equivalently (Definition 12.12), HHH is an RKHS exactly when every evaluation functional f↦f(x)f\mapsto f(x)f↦f(x) is bounded on HHH.

Formalization targets

Goal (Theorem 12.11, the Moore-Aronszajn theorem)

Given any PSD kernel function KKK on any set XXX, there is a Hilbert space HHH (embedded into functions on XXX) in which KKK satisfies the reproducing property (12.3) — and this Hilbert space is unique: any two Hilbert spaces with this property for the same KKK are linearly isometric via an isometry intertwining their embeddings into functions on XXX.

Milestones

  • Theorem 12.5 (Riesz representation). Every bounded linear functional on a Hilbert space HHH has a unique representer g∈Hg\in Hg∈H: L(f)=⟨f,g⟩HL(f)=\langle f,g\rangle_HL(f)=⟨f,g⟩H​ for all fff. Used inside the proof of Theorem 12.13 to produce the representer RxR_xRx​ of each evaluation functional.
  • Theorem 12.13 (the converse correspondence). Given any Hilbert space HHH of functions on XXX in which every evaluation functional is bounded, there is a unique PSD kernel KKK satisfying the reproducing property for HHH — completing the Moore-Aronszajn equivalence between PSD kernels and Hilbert spaces with bounded evaluation functionals.
  • Theorem 12.20 (Mercer's theorem). Under compactness of XXX, continuity of KKK, and the Hilbert-Schmidt condition ∫X×XK2 dP dP<∞\int_{X\times X}K^2\,dP\,dP<\infty∫X×X​K2dPdP<∞, the integral operator TK(f)(x)=∫XK(x,z)f(z) dP(z)T_K(f)(x)=\int_XK(x,z)f(z)\,dP(z)TK​(f)(x)=∫X​K(x,z)f(z)dP(z) has an orthonormal eigenbasis (φj)(\varphi_j)(φj​) of L2(X;P)L^2(X;P)L2(X;P) with non-negative eigenvalues (μj)(\mu_j)(μj​), and K(x,z)=∑jμjφj(x)φj(z)K(x,z)=\sum_j\mu_j\varphi_j(x)\varphi_j(z)K(x,z)=∑j​μj​φj​(x)φj​(z), with the series converging absolutely and uniformly.

Significance

Theorem 12.11 is the theorem that makes the entire RKHS apparatus well-posed: every time a statistician writes down a kernel — linear, polynomial, Gaussian — Theorem 12.11 guarantees that a canonical Hilbert space of functions exists in which that kernel reproduces, so that optimizing over "the RKHS associated with KKK" is a well-defined problem, not merely a suggestive shorthand. Theorem 12.13's converse shows the correspondence is exact — the class of kernel-generated Hilbert spaces is exactly the class of function spaces with bounded evaluation, the class relevant to any statistical application that samples a function at finitely many points. Together, these two results are the foundation the book's own later chapters build directly on: Chapter 13's nonparametric least-squares oracle inequality, and Chapter 14's kernel density estimation, both work by optimizing over an RKHS and are only well-posed because of this correspondence. Mercer's theorem, in turn, is what connects the RKHS viewpoint back to the earlier feature-map viewpoint of Chapter 12.2.2 (Eq. 12.2): the eigenfunctions (μjφj)j(\sqrt{\mu_j}\varphi_j)_j(μj​​φj​)j​ give an explicit feature map into ℓ2(N)\ell^2(\mathbb N)ℓ2(N) realizing KKK, and its expansion is what later underlies the book's discussion of kernel PCA and of RKHS balls as ellipsoids in ℓ2(N)\ell^2(\mathbb N)ℓ2(N)-coordinates.

Difficulty

The formalization difficulty is concentrated in getting the type of the existence-and- uniqueness claim right, not in any single hypothesis. A Hilbert space is not naturally a subtype of a fixed ambient space in Lean, so "the Hilbert space HHH" of Theorem 12.11 is formalized as an abstract type together with its own NormedAddCommGroup/InnerProductSpace ℝ/CompleteSpace instances, connected to "a space of functions on XXX" via an injective linear embedding into X→RX\to\mathbb RX→R — and uniqueness must then be stated as an isometric equivalence between any two witnessing Hilbert spaces that respects this embedding, the faithful rendering of the book's own proof, which literally shows two candidate Hilbert spaces are equal as sets of functions. A second subtlety is keeping Theorem 12.11's hypotheses (a bare PSD kernel, no topology on XXX) cleanly separated from Mercer's theorem's additional compactness, continuity and measure-theoretic apparatus — the two theorems are frequently conflated informally, but the book is explicit that Theorem 12.11 needs none of Mercer's structure.

Formalization scope

XXX is an unconstrained Type* for Theorem 12.5, 12.11 and 12.13 — no topology, matching the book's own generality. Mercer's theorem (Theorem 12.20) additionally requires [MetricSpace X] [CompactSpace X] [MeasurableSpace X] [BorelSpace X] and a finite measure P, matching its own compactness/continuity/measure-theoretic hypotheses exactly, never applied outside that scope. The integral operator TKT_KTK​ of Eq. (12.11a) is presented as an abstract linear map on Lp ℝ 2 P tied to the defining integral formula via an explicit hypothesis, rather than constructed as a def, since constructing it as a genuine well-defined operator (needing integrability and a.e.-measurability arguments) is proof content, not definitional content, and this mission's definitions file is sorry-free by convention. Mercer's orthonormal-basis index type is existentially quantified over a countable ι (∃ (ι : Type) (_ : Countable ι), ...) rather than fixed to ℕ, since L²(X;P) can be finite-dimensional for finite X (Example 12.18/12.21), where no infinite orthonormal basis exists; the uniform-convergence conjunct is correspondingly quantified over every bijection e : ℕ ≃ ι (vacuous when ι is finite, a genuine order-independent claim when ι is countably infinite). A trivializing formalization of this chapter would state only existence in Theorem 12.11 and drop uniqueness (explicitly warned against by this chapter's own brief), or state Mercer's convergence merely pointwise or in L2L^2L2 rather than absolutely and uniformly; this mission avoids both. Out of scope: the constructive proof detail of Theorem 12.11 (the explicit span-and-complete construction is proof content, not part of the statement), the chapter's worked kernel examples (linear, polynomial, Gaussian kernels, Examples 12.7–12.9), and the further consequences of Mercer's theorem (Corollary 12.26 on RKHS-ball ellipsoids, the feature-map connection of Eq. 12.14) — all natural follow-on work for a future mission on kernel-based nonparametric regression (Chapter 13, mission 13-nonparametric-ls), which restates whatever RKHS objects it needs locally rather than importing this mission's draft, per this book's series-wide convention.

Selected references

  • Wainwright, M. J. High-Dimensional Statistics: A Non-Asymptotic Viewpoint. Cambridge University Press, 2019. Chapter 12. DOI: 10.1017/9781108627771.
  • Aronszajn, N. "Theory of reproducing kernels." Transactions of the American Mathematical Society, 68(3), 1950, 337–404.
  • Mercer, J. "Functions of positive and negative type, and their connection with the theory of integral equations." Philosophical Transactions of the Royal Society A, 209, 1909, 415–446.
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Machine LearningProbabilityStatistics·Captain: mikedeng1

High-Dimensional Statistics XII: An Oracle Inequality for Nonparametric Least SquaresTextbook

Motivation

Regression is usually taught with a fixed parametric model: linear regression fits a ddd-dimensional coefficient vector, and the estimation error is controlled by d/nd/nd/n. Many regression problems in practice have no such finite-dimensional description — the regressor is only known to be, say, convex, monotone, or smooth, and the estimator is a least-squares fit over the (infinite-dimensional) set of functions with that shape. This is nonparametric regression, and the basic question is the same as in the parametric case: how close is the fitted function to the truth, as a function of the sample size nnn? Answering it requires replacing "dimension" with a genuinely functional notion of complexity, since an infinite- dimensional function class can still be small enough to estimate well (a Sobolev ball) or too large to estimate at all. The theory in this mission, due to van de Geer and developed in Chapter 13 of Wainwright (High-Dimensional Statistics: A Non-Asymptotic Viewpoint, Cambridge University Press, 2019), gives a single non-asymptotic template — the localized Gaussian complexity — that answers this question for an arbitrary star-shaped function class, and recovers the familiar parametric and Sobolev/RKHS rates as special cases.

Setting

Fix nnn design points x1,…,xnx_1,\dots,x_nx1​,…,xn​ in an arbitrary covariate space X\mathcal XX (fixed, not random — this is the fixed-design setting) and observe

yi=f∗(xi)+σwi,i=1,…,n,y_i = f^*(x_i) + \sigma w_i, \qquad i = 1,\dots,n,yi​=f∗(xi​)+σwi​,i=1,…,n,

where f∗f^*f∗ is the unknown regression function, σ>0\sigma > 0σ>0 is a known noise level, and w1,…,wnw_1,\dots,w_nw1​,…,wn​ are i.i.d. standard Gaussian. Given a class FFF of candidate functions, the nonparametric least-squares estimate is any minimizer

f^n∈arg⁡min⁡f∈F 1n∑i=1n(yi−f(xi))2.\hat f_n \in \arg\min_{f\in F}\ \frac1n\sum_{i=1}^n \big(y_i - f(x_i)\big)^2.f^​n​∈argf∈Fmin​ n1​i=1∑n​(yi​−f(xi​))2.

Error is measured in the empirical (design-dependent) seminorm ∥g∥n2:=1n∑i=1ng(xi)2\|g\|_n^2 := \frac1n\sum_{i=1}^n g(x_i)^2∥g∥n2​:=n1​∑i=1n​g(xi​)2. A class HHH of functions is star-shaped if h∈Hh\in Hh∈H and α∈[0,1]\alpha\in[0,1]α∈[0,1] together imply αh∈H\alpha h \in Hαh∈H — every convex class containing the origin has this property, and it is the minimal structural assumption under which the theory below applies. For a star-shaped class HHH and radius δ>0\delta>0δ>0, the local Gaussian complexity

Gn(δ;H):=Ew[ sup⁡h∈H, ∥h∥n≤δ ∣1n∑i=1nwih(xi)∣ ]G_n(\delta; H) := \mathbb E_w\Big[\ \sup_{h\in H,\ \|h\|_n\le\delta}\ \Big|\tfrac1n \sum_{i=1}^n w_i h(x_i)\Big|\ \Big]Gn​(δ;H):=Ew​[ h∈H, ∥h∥n​≤δsup​ ​n1​i=1∑n​wi​h(xi​)​ ]

measures how much a mean-zero Gaussian process can be made to look like a member of HHH restricted to the ball of radius δ\deltaδ. A critical radius δn\delta_nδn​ is any positive solution of Gn(δ;H)/δ≤δ/(2σ)G_n(\delta;H)/\delta \le \delta/(2\sigma)Gn​(δ;H)/δ≤δ/(2σ); by Lemma 13.6, δ↦Gn(δ;H)/δ\delta\mapsto G_n(\delta;H)/\deltaδ↦Gn​(δ;H)/δ is non-increasing on HHH star-shaped, so this inequality always has a smallest positive solution.

Formalization targets

Lemma 13.6. For any star-shaped HHH, δ↦Gn(δ;H)/δ\delta \mapsto G_n(\delta;H)/\deltaδ↦Gn​(δ;H)/δ is non-increasing on (0,∞)(0,\infty)(0,∞), and consequently Gn(δ;H)/δ≤cδG_n(\delta;H)/\delta \le c\deltaGn​(δ;H)/δ≤cδ has a smallest positive solution for every c>0c>0c>0.

Theorem 13.5 (special case, f∗∈Ff^*\in Ff∗∈F).

P[∥f^n−f∗∥n2≥16 tδn]≤e−ntδn/(2σ2)for all t≥δn.\mathbb P\big[\|\hat f_n - f^*\|_n^2 \ge 16\,t\delta_n\big] \le e^{-nt\delta_n/(2\sigma^2)} \qquad \text{for all } t \ge \delta_n.P[∥f^​n​−f∗∥n2​≥16tδn​]≤e−ntδn​/(2σ2)for all t≥δn​.

Theorem 13.13 (goal — general oracle inequality, f∗f^*f∗ not assumed in FFF). With δn\delta_nδn​ solving the critical inequality for ∂F:=F−F\partial F := F - F∂F:=F−F, there are universal constants (c0,c1,c2)(c_0,c_1,c_2)(c0​,c1​,c2​) such that for all t≥δnt\ge\delta_nt≥δn​,

∥f^n−f∗∥n2≤inf⁡γ∈(0,1)[1+γ1−γ∥f−f∗∥n2+c0γ(1−γ)tδn]for all f∈F,\|\hat f_n-f^*\|_n^2 \le \inf_{\gamma\in(0,1)}\left[\frac{1+\gamma}{1-\gamma}\|f-f^*\|_n^2 +\frac{c_0}{\gamma(1-\gamma)}t\delta_n\right]\quad\text{for all }f\in F,∥f^​n​−f∗∥n2​≤γ∈(0,1)inf​[1−γ1+γ​∥f−f∗∥n2​+γ(1−γ)c0​​tδn​]for all f∈F,

with probability at least 1−c1e−c2ntδn/σ21-c_1e^{-c_2nt\delta_n/\sigma^2}1−c1​e−c2​ntδn​/σ2. The goal is deliberately the statement with unresolved universal constants and an infimum over γ\gammaγ, rather than any single instantiated bound, so the target survives sharper constant tracking.

Significance

Theorem 13.13 is the "master" result behind essentially every concrete rate in the chapter: orthogonal series regression, convex/monotone regression, and (via the KRR specialization of Section 13.4) kernel ridge regression rates for Sobolev and Gaussian-kernel classes are all obtained by bounding GnG_nGn​ for a particular FFF and reading off δn\delta_nδn​. Its value is that it isolates exactly the one place where the geometry of FFF enters — the local Gaussian complexity — while the probabilistic argument (a peeling/chaining argument controlling a localized empirical process) is generic. Formalizing it produces, for the first time on the platform, the statement-level infrastructure (star-shaped classes, local Gaussian complexity, critical radius) that any future mission on a concrete nonparametric-regression rate — kernel ridge regression, convex regression, isotonic regression — can specialize, without re-deriving the oracle inequality from scratch. The proof itself (concentration of Gaussian complexity via Borell-TIS/Gaussian comparison plus a peeling argument over dyadic scales) is not attempted here; only the statement is formalized, as a draft goal for future proof contributions.

Difficulty

The naive route to Theorem 13.13 is to bound ∥f^n−f∗∥n\|\hat f_n - f^*\|_n∥f^​n​−f∗∥n​ pointwise via the basic inequality 12∥f^n−f∗∥n2≤σn∑iwi(f^n(xi)−f∗(xi))\tfrac12\|\hat f_n-f^*\|_n^2 \le \tfrac{\sigma}{n}\sum_i w_i(\hat f_n(x_i)-f^*(x_i))21​∥f^​n​−f∗∥n2​≤nσ​∑i​wi​(f^​n​(xi​)−f∗(xi​)) and then bound the right side by σ Gn(δ;∂F)\sigma\,G_n(\delta;\partial F)σGn​(δ;∂F) for δ=∥f^n−f∗∥n\delta = \|\hat f_n-f^*\|_nδ=∥f^​n​−f∗∥n​ — but δ\deltaδ is itself random (it depends on the estimate), so this is circular: the bound on the right depends on the very quantity being bounded. The chapter's actual argument resolves this with a peeling device: partition the event space by which dyadic annulus ∥f^n−f∗∥n\|\hat f_n-f^*\|_n∥f^​n​−f∗∥n​ falls into, and apply a uniform (non-circular) bound on each annulus separately via Gaussian concentration, summing a geometric series of tail probabilities. This is the step every first attempt misses, and it is why the local Gaussian complexity — rather than the simpler global complexity of Chapter 4/5 — is the right object: localizing to radius δ\deltaδ is what makes the per-annulus bound tight enough for the final sum to converge.

Formalization scope

Design points are an arbitrary type X (no topology or metric structure is needed for the statements themselves); the least-squares estimate is represented as a Prop (IsLeastSquaresEstimate) picking out any function achieving the empirical minimum, matching the book's "any minimizer" phrasing rather than assuming uniqueness. The local Gaussian complexity is defined as an expectation over an explicit i.i.d.-standard-Gaussian noise vector on an abstract probability space, with the inner supremum taken over the subtype of the radius-restricted slice of the class — this is well-defined (not the junk value 0 of an unbounded Set ℝ supremum) whenever the slice is nonempty, which holds automatically for any nonempty star-shaped class (taking α=0\alpha=0α=0 exhibits 000 in the class). Since neither X nor H carries a topology, separability or countability constraint, SatisfiesCriticalInequality adds an explicit Integrable hypothesis on that same supremum (added in revision), guarding against Mathlib's Bochner integral silently returning the junk value 0 for a non-measurable integrand — a value that would otherwise trivially satisfy the critical inequality for every positive δ, regardless of the function class's actual local complexity. The trivializing formalization to rule out here is stating Theorem 13.13's universal constants after the quantification over the function class and sample size, which would let (c0,c1,c2)(c_0,c_1,c_2)(c0​,c1​,c2​) secretly depend on the instance and make the "universal" claim vacuous; this mission places the constant quantifiers first, before the class, design and noise data they must not depend on. A complete downstream development would add: the concentration-of-Gaussian-complexity step (Borell–TIS or a comparable tail bound), the peeling argument, and the metric-entropy / Dudley-integral machinery of Section 13.2.1 for bounding GnG_nGn​ explicitly on concrete classes (Sobolev balls, RKHS balls) — none of which is attempted here.

Selected references

  • M. Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint, Cambridge University Press, 2019, Chapter 13. https://doi.org/10.1017/9781108627771
  • S. van de Geer, Empirical Processes in M-Estimation, Cambridge University Press, 2000.
  • S. van de Geer, "Estimating a regression function," Annals of Statistics, 18(2):907-924, 1990. https://doi.org/10.1214/aos/1176347627
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Machine LearningProbabilityStatistics·Captain: mikedeng1

High-Dimensional Statistics XIII: A Localized Uniform LawTextbook

Motivation

Every consistency guarantee for an empirical-risk-minimization procedure — the Lasso, kernel ridge regression, maximum likelihood — ultimately rests on relating an empirical average to its population expectation, uniformly over the class of candidate functions or parameters being searched. Chapter 4 established the classical form of this connection: a uniform law of large numbers, bounding sup⁡f∈F∣∥f∥n2−∥f∥22∣\sup_{f\in F}|\|f\|_n^2-\|f\|_2^2|supf∈F​∣∥f∥n2​−∥f∥22​∣ by an absolute quantity governed by the (unlocalized) complexity of FFF. Such a bound is often wasteful: it treats a function with small population norm the same as one with large population norm, when intuitively the empirical and population norms of a small function should already agree closely. This mission formalizes the sharper, localized form of this uniform law — the same localization principle Chapter 13 used for nonparametric least squares, now applied directly to the empirical-versus-population norm comparison itself, giving relative rather than absolute control and recovering optimal convergence rates that the unlocalized theory misses.

Setting

Fix a probability distribution PPP over a covariate space XXX and nnn i.i.d. samples x1,…,xn∼Px_1,\dots,x_n\sim Px1​,…,xn​∼P. For f:X→Rf:X\to\mathbb Rf:X→R, the population norm is ∥f∥22:=∫Xf(x)2 P(dx)\|f\|_2^2:=\int_Xf(x)^2\,P(dx)∥f∥22​:=∫X​f(x)2P(dx) and the empirical norm is ∥f∥n2:=1n∑i=1nf(xi)2\|f\|_n^2:=\frac1n\sum_{i=1}^nf(x_i)^2∥f∥n2​:=n1​∑i=1n​f(xi​)2; by linearity of expectation, E[∥f∥n2]=∥f∥22\mathbb E[\|f\|_n^2]=\|f\|_2^2E[∥f∥n2​]=∥f∥22​, so the question is how tightly ∥f∥n2\|f\|_n^2∥f∥n2​ concentrates around ∥f∥22\|f\|_2^2∥f∥22​, uniformly over a function class FFF. A class FFF is star-shaped around the origin if f∈F,α∈[0,1]  ⟹  αf∈Ff\in F,\alpha\in[0,1]\implies\alpha f\in Ff∈F,α∈[0,1]⟹αf∈F, and bbb-uniformly bounded if ∥f∥∞≤b\|f\|_\infty\le b∥f∥∞​≤b for every f∈Ff\in Ff∈F. The relevant complexity measure is the population localized Rademacher complexity

Rn(δ;F):=Eε,x[ sup⁡f∈F, ∥f∥2≤δ ∣1n∑i=1nεif(xi)∣ ],R_n(\delta;F) := \mathbb E_{\varepsilon,x}\Big[\ \sup_{f\in F,\ \|f\|_2\le\delta}\ \Big| \tfrac1n\sum_{i=1}^n\varepsilon_if(x_i)\Big|\ \Big],Rn​(δ;F):=Eε,x​[ f∈F, ∥f∥2​≤δsup​ ​n1​i=1∑n​εi​f(xi​)​ ],

where ε1,…,εn\varepsilon_1,\dots,\varepsilon_nε1​,…,εn​ are i.i.d. Rademacher signs independent of the samples — note that, unlike Chapter 13's Gaussian complexity for fixed design points, this expectation integrates out the randomness of the samples themselves, since this chapter treats {xi}\{x_i\}{xi​} as genuinely random throughout. A critical radius δn\delta_nδn​ is any positive solution of Rn(δ;F)≤δ2/bR_n(\delta;F)\le\delta^2/bRn​(δ;F)≤δ2/b.

Formalization targets

Theorem 14.1 (goal). Given FFF star-shaped and bbb-uniformly bounded, and δn\delta_nδn​ solving the critical inequality, for any t≥δnt\ge\delta_nt≥δn​,

∣∥f∥n2−∥f∥22∣≤12∥f∥22+t22for all f∈F,\Big|\|f\|_n^2-\|f\|_2^2\Big|\le\frac12\|f\|_2^2+\frac{t^2}2 \qquad\text{for all }f\in F,​∥f∥n2​−∥f∥22​​≤21​∥f∥22​+2t2​for all f∈F,

with probability at least 1−c1e−c2nt2/b21-c_1e^{-c_2nt^2/b^2}1−c1​e−c2​nt2/b2; and if additionally nδn2≥2c2log⁡(4log⁡(1/δn))n\delta_n^2\ge\frac2{c_2}\log(4\log(1/\delta_n))nδn2​≥c2​2​log(4log(1/δn​)),

∣∥f∥n−∥f∥2∣≤c0δnfor all f∈F,\big|\|f\|_n-\|f\|_2\big|\le c_0\delta_n \qquad\text{for all }f\in F,​∥f∥n​−∥f∥2​​≤c0​δn​for all f∈F,

with probability at least 1−c1′e−c2′nδn2/b21-c_1'e^{-c_2'n\delta_n^2/b^2}1−c1′​e−c2′​nδn2​/b2.

Significance

Theorem 14.1 is the technical engine behind two of the book's other sharp results: Example 14.2's derivation of the optimal n−1/2n^{-1/2}n−1/2 rate for bounded quadratic function classes (where the unlocalized analogue of this theorem only achieves the slower n−1/4n^{-1/4}n−1/4 rate), and, more broadly, every later argument in the book that needs to translate an empirical-norm guarantee (as produced directly by an M-estimator's optimality, e.g. Chapter 13's nonparametric least-squares bounds) into a population-norm guarantee, or vice versa. The gap between the "absolute" uniform law of Chapter 4 and the "relative" one here is exactly the difference between a bound that is only informative for functions of order-one population norm, and one that remains sharp arbitrarily close to the origin — which is precisely where a consistent estimator's error eventually lives. Formalizing the statement produces, for the first time on the platform, the localized-Rademacher-complexity vocabulary at the population level (as opposed to Chapter 13's fixed-design Gaussian-complexity version), reusable by any future mission needing to pass between empirical and population norms.

Difficulty

The naive approach — apply Hoeffding's inequality to ∣∥f∥n2−∥f∥22∣|\|f\|_n^2-\|f\|_2^2|∣∥f∥n2​−∥f∥22​∣ for a fixed fff, then union-bound (or apply the unlocalized Rademacher-complexity uniform law of Chapter 4) over FFF — gives a bound whose complexity term does not shrink as ∥f∥2→0\|f\|_2\to0∥f∥2​→0, since it uses the complexity of all of FFF regardless of a given function's own size. This is exactly the sub-optimality Example 14.2 exhibits concretely: the naive bound gives rate n−1/4n^{-1/4}n−1/4 where the truth is n−1/2n^{-1/2}n−1/2. The fix is not merely technical bookkeeping — it requires a genuine peeling argument over dyadic norm-scales (exactly as in Chapter 13's proof of Theorem 13.13), applying the localized complexity Rn(δ;F)R_n(\delta;F)Rn​(δ;F) at the scale δ=∥f∥2\delta=\|f\|_2δ=∥f∥2​ appropriate to each individual fff, and controlling the resulting geometric sum of tail probabilities across scales. A reader's first instinct — bound ∥f∥2\|f\|_2∥f∥2​ in terms of ∥f∥n\|f\|_n∥f∥n​ and substitute — is circular, since ∥f∥n\|f\|_n∥f∥n​ is itself the random quantity being controlled.

Formalization scope

The covariate space X carries an arbitrary MeasurableSpace structure (no topology needed for the statement); the sample sequence and the Rademacher signs are both represented as families of measurable functions on a shared probability space Ω, with their joint independence stated as a single IndepFun between the two vector-valued sequences (rather than building a combined-index iIndepFun), since it is the two sequences — not each pair of individual variables — whose independence the book invokes. The two conclusions of Theorem 14.1 are stated as a conjunction with the second gated behind its own extra hypothesis, never collapsed into a single implication, since the book's own statement keeps them syntactically and logically distinct (the second requires a strictly stronger and additional condition on top of the first's). The universal constants (c1,c2,c0,c1',c2') are quantified before every instance object, so they cannot secretly depend on the function class, sample size, or radius. Every f ∈ F is required measurable (hF_meas, added in revision): the book's own framing implicitly restricts to measurable, square-integrable f throughout (p. 454), and without this hypothesis the population norm popNormSq, which appears directly in the goal's conclusion, could silently take Mathlib's Bochner-integral junk value 0 for a non-measurable, pointwise-bounded member of a star-shaped, uniformly-bounded F. The trivializing formalization ruled out here is stating the localization constraint at the empirical rather than population norm in popRademacherComplexity — this chapter's whole point (contrast Chapter 13's Gn, correctly localized at the empirical norm since there the design is fixed) is that Rn(δ;F)R_n(\delta;F)Rn​(δ;F)'s localization is a population-level object, precisely because the samples are random here. Welcome future contributions: Corollary 14.3's covering-number sufficient condition for the empirical version of the critical inequality, and Theorem 14.20's Lipschitz/strongly-convex cost-function uniform law, both deferred from this mission (see STATUS.md) as they need substantial additional apparatus (metric entropy integrals; cost functions and strong convexity) beyond what Theorem 14.1 itself requires.

Selected references

  • M. Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint, Cambridge University Press, 2019, Chapter 14. https://doi.org/10.1017/9781108627771
  • P. Bartlett, O. Bousquet and S. Mendelson, "Local Rademacher complexities," Annals of Statistics, 33(4):1497-1537, 2005. https://doi.org/10.1214/009053605000000282
  • V. Koltchinskii, "Local Rademacher complexities and oracle inequalities in risk minimization," Annals of Statistics, 34(6):2593-2656, 2006. https://doi.org/10.1214/009053606000001019
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Machine LearningProbabilityRandom Matrix Theory+1·Captain: mikedeng1

High-Dimensional Statistics V: Thresholding-Based Covariance EstimationTextbook

Motivation

Estimating a d×dd\times dd×d covariance matrix Σ\SigmaΣ from nnn samples is a canonical high-dimensional problem: the natural estimator, the sample covariance Σ^\hat\SigmaΣ^, is consistent in operator norm only when n≳dn\gtrsim dn≳d, which fails outright in the regime d≫nd\gg nd≫n common to modern applications. When Σ\SigmaΣ is additionally known to be sparse — few nonzero entries per row — a simple fix restores consistency even when d≫nd\gg nd≫n: threshold every entry of Σ^\hat\SigmaΣ^ below a data-dependent level to zero. This mission formalizes the matrix concentration machinery behind that fix and the resulting guarantee, following Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint (Cambridge University Press, 2019), Chapter 6.

Setting

For a random matrix QQQ, the matrix variance is var(Q):=E[Q2]−(E[Q])2\mathrm{var}(Q):=\mathbb E[Q^2]-(\mathbb E[Q])^2var(Q):=E[Q2]−(E[Q])2, and the Loewner order A⪯BA\preceq BA⪯B on symmetric matrices means B−AB-AB−A is positive semidefinite. A zero-mean symmetric random matrix QQQ satisfies Bernstein's condition (Definition 6.10) with parameter b>0b>0b>0 if E[Qj]⪯12j! bj−2var(Q)\mathbb E[Q^j]\preceq\tfrac12 j!\,b^{j-2}\mathrm{var}(Q)E[Qj]⪯21​j!bj−2var(Q) for j=3,4,…j=3,4,\dotsj=3,4,… — the matrix analogue of the scalar Bernstein condition of Chapter 2. The operator (spectral) norm ∣ ⁣∣ ⁣∣M∣ ⁣∣ ⁣∣2|\!|\!|M|\!|\!|_2∣∣∣M∣∣∣2​ is MMM's largest singular value.

Given a threshold λ>0\lambda>0λ>0, the hard-thresholding operator is Tλ(u):=u⋅1[∣u∣>λ]T_\lambda(u):=u\cdot \mathbb 1[|u|>\lambda]Tλ​(u):=u⋅1[∣u∣>λ], extended entrywise to matrices (Eq. (6.52)). A covariance matrix Σ\SigmaΣ's sparsity pattern is captured by its adjacency matrix Ajℓ:=1[Σjℓ≠0]A_{j\ell}:=\mathbb 1[\Sigma_{j\ell}\neq0]Ajℓ​:=1[Σjℓ​=0] (p. 181); ∣ ⁣∣ ⁣∣A∣ ⁣∣ ⁣∣2≤d|\!|\!|A|\!|\!|_2\le d∣∣∣A∣∣∣2​≤d always, with equality only when Σ\SigmaΣ has no zero entries, and ∣ ⁣∣ ⁣∣A∣ ⁣∣ ⁣∣2≤s|\!|\!|A|\!|\!|_2\le s∣∣∣A∣∣∣2​≤s whenever Σ\SigmaΣ has at most sss nonzero entries per row.

Formalization targets

Goal — Theorem 6.23 (thresholding-based covariance estimation)

Let {xi}i=1n\{x_i\}_{i=1}^n{xi​}i=1n​ be i.i.d. zero-mean random vectors with covariance Σ\SigmaΣ, each coordinate sub-Gaussian with parameter at most σ\sigmaσ. If n>log⁡dn>\log dn>logd, then for any δ>0\delta>0δ>0, the thresholded sample covariance Tλn(Σ^)T_{\lambda_n}(\hat\Sigma)Tλn​​(Σ^) with λn/σ2=8log⁡d/n+δ\lambda_n/\sigma^2 = 8\sqrt{\log d/n}+\deltaλn​/σ2=8logd/n​+δ satisfies

P[ ∣ ⁣∣ ⁣∣Tλn(Σ^)−Σ∣ ⁣∣ ⁣∣2≥2∣ ⁣∣ ⁣∣A∣ ⁣∣ ⁣∣2λn ]  ≤  8e−n16min⁡{δ,δ2}.\mathbb P\big[\,|\!|\!|T_{\lambda_n}(\hat\Sigma)-\Sigma|\!|\!|_2 \ge 2|\!|\!|A|\!|\!|_2\lambda_n\,\big] \;\le\; 8e^{-\frac{n}{16}\min\{\delta,\delta^2\}}.P[∣∣∣Tλn​​(Σ^)−Σ∣∣∣2​≥2∣∣∣A∣∣∣2​λn​]≤8e−16n​min{δ,δ2}.

The error scales with the graph sparsity ∣ ⁣∣ ⁣∣A∣ ⁣∣ ⁣∣2|\!|\!|A|\!|\!|_2∣∣∣A∣∣∣2​, not with ddd directly — the whole point of thresholding when the ambient dimension is much larger than the sample size.

Milestone — Theorem 6.17 (the matrix Bernstein bound)

For independent, zero-mean, symmetric random matrices {Qi}\{Q_i\}{Qi​} satisfying Bernstein's condition with parameter bbb,

P[1n∣ ⁣∣ ⁣∣∑i=1nQi∣ ⁣∣ ⁣∣2≥δ]  ≤  2 rank(∑i=1nvar(Qi))exp⁡(−nδ22(σ2+bδ)).\mathbb P\Big[\frac1n\Big|\!\Big|\!\Big|\sum_{i=1}^n Q_i\Big|\!\Big|\!\Big|_2 \ge \delta\Big] \;\le\; 2\,\mathrm{rank}\Big(\sum_{i=1}^n\mathrm{var}(Q_i)\Big)\exp\Big(-\frac{n\delta^2}{2(\sigma^2+b\delta)}\Big).P[n1​​​​i=1∑n​Qi​​​​2​≥δ]≤2rank(i=1∑n​var(Qi​))exp(−2(σ2+bδ)nδ2​).

This is the general matrix concentration tool the whole chapter builds toward; Theorem 6.23 is one of its corollaries.

Milestone — Eq. (6.54) (the deterministic thresholding bound)

For any λn\lambda_nλn​ with ∥Σ^−Σ∥max⁡≤λn\|\hat\Sigma-\Sigma\|_{\max}\le\lambda_n∥Σ^−Σ∥max​≤λn​, ∣ ⁣∣ ⁣∣Tλn(Σ^)−Σ∣ ⁣∣ ⁣∣2≤2∣ ⁣∣ ⁣∣A∣ ⁣∣ ⁣∣2λn|\!|\!|T_{\lambda_n}(\hat\Sigma)-\Sigma|\!|\!|_2\le2|\!|\!|A|\!|\!|_2\lambda_n∣∣∣Tλn​​(Σ^)−Σ∣∣∣2​≤2∣∣∣A∣∣∣2​λn​ — a purely deterministic fact, with no probability involved, that reduces Theorem 6.23's proof to a single probabilistic input: controlling ∥Σ^−Σ∥max⁡\|\hat\Sigma-\Sigma\|_{\max}∥Σ^−Σ∥max​.

Significance

Theorem 6.17 is the workhorse of the whole chapter: besides Theorem 6.23, it also underlies Corollary 6.20's operator-norm bound for the unstructured sample covariance matrix (used in turn for the two example ensembles in Section 6.4.5), by taking Qi:=xixiT−ΣQ_i:=x_ix_i^T-\SigmaQi​:=xi​xiT​−Σ. Theorem 6.23 itself is the standard justification for thresholding-based covariance estimators used throughout high-dimensional statistics whenever the sparsity pattern of Σ\SigmaΣ, though unknown, is believed to be structured.

Formalizing it. No faithful prior art exists on the platform for the matrix Bernstein bound or covariance thresholding (a fresh search for "matrix Bernstein," "Bernstein condition matrix," "thresholding covariance," and "sparse covariance" returned no hits). The existing RademacherWigner.* items formalize spectral-edge and empirical-spectral-distribution bounds for the Wigner ensemble specifically (a symmetric matrix with i.i.d. entries) — a narrower, different random-matrix model from the general Bernstein-condition matrices this chapter treats, and not reused here. All three theorems are drafted as open goals (:= by sorry).

Difficulty

The naive approach to a matrix tail bound — apply the scalar Chernoff/Bernstein technique directly to the operator norm — fails because the operator norm is not a linear functional of QQQ, so the scalar moment generating function bound does not translate directly. The resolution (Lemma 6.13, not itself part of this mission) instead bounds the trace of the matrix exponential of the sum, which is linear-algebraically tractable via the Golden–Thompson-type inequality and the union bound over the (at most rank(Vˉ)\mathrm{rank}(\bar V)rank(Vˉ)) nonzero eigenvalue directions of the aggregate variance Vˉ=∑ivar(Qi)\bar V=\sum_i\mathrm{var}(Q_i)Vˉ=∑i​var(Qi​) — this is exactly why the bound's prefactor is rank(Vˉ)\mathrm{rank}(\bar V)rank(Vˉ), not the ambient dimension ddd: a low-rank aggregate variance (e.g. from a highly structured collection of matrices) yields a much tighter bound than a naive union bound over all ddd eigen-directions would. Theorem 6.23's own difficulty is entirely in the reduction to Theorem 6.17 plus Eq. (6.54): checking that Qi:=xixiT−ΣQ_i:=x_ix_i^T-\SigmaQi​:=xi​xiT​−Σ satisfies the Bernstein condition with the stated parameters, and that ∥Σ^−Σ∥max⁡\|\hat\Sigma-\Sigma\|_{\max}∥Σ^−Σ∥max​ concentrates at the stated rate via a union bound over the O(d2)O(d^2)O(d2) matrix entries.

Formalization scope

"Symmetric" is realized via Mathlib's Matrix.IsSymm; the Loewner order via (B-A).PosSemidef. The matrix moment generating function itself (ΨQ(λ):=E[e^{λQ}]) is not formalized, since none of this mission's three theorem statements need it directly — Bernstein's condition (Definition 6.10) is stated purely in terms of polynomial moments E[Qj]\mathbb E[Q^j]E[Qj], avoiding the substantial extra machinery (Mathlib's NormedSpace.exp for matrices) that a faithful matrix-exponential definition would require, at no cost to faithfulness for the three statements actually drafted.

Independence of {Qi}\{Q_i\}{Qi​}/{xi}\{x_i\}{xi​} is realized via Mathlib's iIndepFun; this required adding a local MeasurableSpace (Matrix (Fin d) (Fin d) ℝ) instance in the workspace, since Matrix is a def, not an abbrev, over the underlying Pi type, so Lean's instance search does not automatically find the Pi-type MeasurableSpace instance for it. "Identically distributed" is realized via Mathlib's IdentDistrib against a fixed reference index. "Each component sub-Gaussian" is restated locally as an explicit MGF bound at the reference index, per this book's cross-chapter rule against importing another chapter's draft definitions.

If a statement admits a trivializing formalization: the rank(...) prefactor of Theorem 6.17 is kept exactly, not replaced by the ambient dimension ddd (which would be a strictly weaker, non-trivializing but unfaithful simplification, since the bound's whole point is that rank(...) ≤ d can be much smaller). ‖·‖_max and opNorm at d=0 return Mathlib's junk value 0 (harmless: no matrix entries or singular values exist at that degenerate size either).

Out of scope for this mission: Theorem 6.15 (the sub-Gaussian-tail matrix concentration result that precedes Theorem 6.17 in the same section) and Corollary 6.20 (the unstructured covariance-estimation corollary) — both natural follow-on work, cut for this chunk's time budget; see STATUS.md.

Selected references

  • M. J. Wainwright, High-Dimensional Statistics: A Non-Asymptotic Viewpoint, Cambridge University Press, 2019. DOI: 10.1017/9781108627771. Chapter 6.
  • J. A. Tropp, "User-friendly tail bounds for sums of random matrices," Foundations of Computational Mathematics, 12(4):389–434, 2012.
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